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Atomic Absorption and Emission Spectra
may exhibit a continuum, or may have superposed on the continuum bright lines (an emission spectrum) or dark lines (an absorption spectrum), as illustrated in
http://csep10.phys.utk.edu/astr162/lect/light/absorption.html
The Physics Zone - Spectroscopy, emission, absorption, Doppler ...
Spectroscopy spectrum, absorption spectrum, emission spectrum, Doppler shift. The Visible Spectrum: Typically, superheated solids
http://www.sciencejoywagon.com/physicszone/lesson/09waves/spectrum/emisndop.htm
Regents Prep- Spectroscopy, emission, absorption, Doppler shift
Spectroscopy spectrum, absorption spectrum, emission spectrum, Doppler shift, The Visible Spectrum: Typically, superheated solids
http://regentsprep.org/Regents/physics/phys05/cspectrum/default.htm
Absorption spectrum
As with the emission spectrum, each element has its own unique absorption spectrum, as the energy levels of different elements differ.
http://theory.uwinnipeg.ca/mod_tech/node152.html
Emission spectrum
This success of the Bohr model in explaining the emission spectra of simple next up previous contents index Next: Absorption spectrum Up: Bohr model Previous
http://theory.uwinnipeg.ca/mod_tech/node151.html
Spectra
An emission spectrum consists of all the radiations emitted by atoms or molecules, whereas in an absorption spectrum, portions of a continuous spectrum (light
http://zebu.uoregon.edu/~js/glossary/spectra.html
GE 70A: Evolution of the Cosmos and Life
Diagram. [2 points] needs to accurately depict the production of either an emission or absorption spectrum. Needs to be understandable.
http://www.physics.ucla.edu/class/02F/GE70A_Morris/homework/Lab2KeyFall02.html
Active Galaxies and Quasars - Emission Spectrum of NGC 4151
careful accounting for the complex absorption that our scanned the wavelengths of strong emission lines in the blocky appearance of the deep infrared spectrum.
http://www.astr.ua.edu/keel/agn/ngc4151sp.html
Absorption Spectra
(Note that the dark lines in an absorption spectrum appear at exactly the same frequencies as the bright lines in the corresponding emission spectrum.).
http://www.colorado.edu/physics/2000/quantumzone/fraunhofer.html
Java Applets
Java Applets We have four Java applets related to light emission and absorption: Example Coloring Applet Emission Spectrum Absorption Spectrum Single Filter Emission We have also developed four Java
http://mc2.cchem.berkeley.edu/Java/
Emission Line Spectrum, Absorption Line Spectrum and Continous Spectrum
7b10.10 Emission Line Spectrum, Absorption Line Spectrum and a Continous Spectrum To show the emission line spectrum for various low pressure gases, an absorption line spectrum from Na, and a
http://www.physics.brown.edu/Studies/Demo/modern/demo/7b1010.htm
http://jersey.uoregon.edu/vlab/elements/Elements.html
you separate the light that is passing through a sample, or reflecting off a sample, you end up with an emission spectrum or absorption spectrum, as opposed to
http://jersey.uoregon.edu/vlab/elements/Elements.html
Uranyl Poster
monochromator fluorimeter (Figure 2). A typical absorption spectrum is shown in Figure 3. Emission and Excitation Spectra. In an emission spectrum, the sample
http://www.wellesley.edu/Chemistry/Flick/uranylposter.html
Molecular Expressions Microscopy Primer: Specialized Microscopy ...
To determine the Emission spectrum of a given fluorochrome, the dye absorption maximum wavelength (usually the same as the excitation maximum) is found and the
http://micro.magnet.fsu.edu/primer/techniques/fluorescence/excitation.html
XCSAO Example 2 Spectrum with Labelled Absorption Lines
Example 2] [Emission summary] [Correlation summary] [Full Spectrum] [Calcium H and K] [Hydrogen alpha] [Spectrum+emission] [Spectrum+absorption] [Spectrum+all
http://tdc-www.harvard.edu/iraf/rvsao/xcsao/ex2/xcsao.ex2sum1m2a.html
GSFC Press Release 99-089
Key to his recent ASCA observation, Nandra said, was the detection of a red-shifted absorption feature in the emission spectrum.
http://www.gsfc.nasa.gov/news-release/releases/1999/99-089.htm
continuous spectrum (emission or absorption)
continuous spectrum(emission or absorption) of: electromagnetic radiation (usually from a ...specified source) is: a spectrum spectrum from a solid or liquid heated to a high temperature. [P8.2] is exemplified: by white light, which
http://www.physics.rdg.ac.uk/units/flap/glossary/cc/cntsspct.htm
Emission Spectrum of Hydrogen
Development of Current Atomic Theory EmissionSpectrum Spectrum Bohr Model of the Atom Wave-Particle Duality Bohr Model vs. ...these photons carries about 171,000 joules of energy, or 171 kJ/mol. Absorption of a mole of photons of red
http://chemed.chem.purdue.edu/genchem/topicreview/bp/ch6/orig_bohr.html
CWRU NSRT About Spectra
An emission spectrum is almost the reverse of an absorption spectrum. In an emission spectrum, you will see just a few sharp lines of color.
http://astrwww.astr.cwru.edu/reference/spectra.html
CHEM 223
Series of Conjugated Dyes 107 Emission Spectrum of a Diatomic Molecule: Nitrogen 108 Absorption Spectrum of Molecular Iodine 109 Emission Spectrum of Molecular
http://www.sas.upenn.edu/chem/courses/Spring2001/chem223.html
A structural probe, materials design, laser properties
There are many areas where access to the enormous amount of information hidden in rare-earth absorption/emission spectrum could be exploited.
http://cfi.lbl.gov/~klinten/thesis/node/node27.html
Spectroscope module
An emission spectrum with a blue line at about 445 nm, a green line at 525 nm, and a red line at 635 nm. When measuring an absorption spectrum, record the
http://chemscape.santafe.cc.fl.us/chemscape/catofp/measurep/spectro/spectrs3.htm
Spectroscopy
The spectrum of an atom or molecule depends on its energy level structure, and absorption spectra are useful for identifying of compounds. Emission.
http://elchem.kaist.ac.kr/vt/chem-ed/spec/spectros.htm
Optics
If the fluorochrome were excited by another wavelength within its absorption spectrum, light emission of the same spectrum would occur but it would not be of
http://www.pmci.unimelb.edu.au/core_facilities/Cytometry/light1.asp
FeH Absorption in the Spectra of Ultra-Cool Dwarfs M. Cushing, J ...
Some regions of the spectra (see below) are completely dominated by FeH absorption. 2000 K while the bottom panel shows an laboratory emission spectrum of FeH
http://irtfweb.ifa.hawaii.edu/Science/cushing.pdf
Taking fingerprints of stars
The more electrons (protons) characterizing an element, the more complex its absorption/emission spectrum. Absorption “lines”.
http://www.cis.rit.edu/class/simg553_03/presentations/line_spectra.ppt
Emission or Absorption spectrum of different gases
Emissionor Absorptionspectrumof different gases Each element has a signature spectrumunique to each element. Helium was first discovered by observing spectrum of Sun Previous slide Next slide Back to first slide View
http://www.bemidjistate.edu/Science/astro/ch4b/tsld007.htm
continuous spectrum (emission or absorption)
continuous spectrum(emission or absorption) of: electromagnetic radiation (usually from a ...specified source) is: a spectrum spectrum from a solid or liquid heated to a high temperature . [P8.2] is exemplified: by white light ,
http://www.physics.reading.ac.uk/units/flap/glossary/cc/cntsspct.htm
Science: Out of This World -- Absorption Spectrum
AbsorptionSpectrum Go to the student menu page Mark this page Help for this Button Main ...Help for Content Pages! Glossary Help EmissionSpectrumWhite Light Spectroscope The Spectrumof Visible Light Emission of
http://www.spacesciencegroup.nsula.edu/lessons/default.asp?theme=light&pagename=absorptionspectrum
SUNKISS THERMOREACTORS®: Emission spectrum of transmitter.
... doesn't support Java. EmissionSpectrumSPECTRUM OF THERMOREACTORS CURING The absorption spectrum of paints, inks, varnish and adhesives, superpose with the spectrum emission of the THERMOREACTORS ® transmitter. To Product
http://www.americanovens.com/home/spectrum1.htm
Muramatsu et al.
Distinctive spectral features in the x-ray emission spectrum of the hydrofullerene are denoted by A and B, and those in the absorption spectrum by C­F. Page 3.
http://alspubs.lbl.gov/AbstractManager/uploads/99114.pdf
Absorption and Emission
produce an absorption line spectrum if it is between you (your telescope+spectrograph) and a continuum light source, and an emission line spectrum if viewed
http://astro.nmsu.edu/~nicole/teaching/ASTR110/lectures/lecture19/slide02.html
Analyzing Spectra
Each element produces a unique set of emission or absorption lines. An emission spectrum involves transitions of electrons from ___________ to ______________
http://www.astro.washington.edu/labs/clearinghouse/labs/Spectanalysis/worksheet.html
Analyzing Spectra
3. For a given atom, will the discrete wavelengths be different depending on whether we are viewing an emission spectrum or an absorption spectrum?
http://www.astro.washington.edu/astro101/CoursePak/specanalysis2.pdf
Email Template
Absorption / Emission spectroscopy (molecular spectroscopy) 107 Emission Spectrum of a Diatomic Molecule: Nitrogen 108 Absorption Spectrum of Molecular Iodine
http://www.sas.upenn.edu/chem/courses/Spring2000/chem223.html
Rami Arieli: The Laser Adventure
Excimer Laser - A gas laser which emits in the UV spectrum. Fluorescence - Emission of light of particular wavelength, as a result of absorption of light at
http://www.phys.ksu.edu/perg/vqm/laserweb/Glossary/Glossary.htm
Astronomy 301: Light
When astronomers look at the sky, we see light coming from three basic forms: continuous spectrum, absorption, and emission spectrum.
http://hoku.as.utexas.edu/~gebhardt/a301f02/lect5.html
PES 105 Light: Spectroscopy and Atoms
[Link to absorption animation]. emission spectrum: If an electron jumps down from a higher level to a lower level, light with a specific energy (wavelength
http://www.uccs.edu/~tchriste/courses/PES105/105lectures/105lecspectro.html
Lecture 1 Outline
o The light that gets absorbed in an absorption spectrum is the same light that is emitted in another direction as an emission spectrum. · Atoms.
http://www.astro.psu.edu/users/gtr/teaching/astro10/spring2002/Lecture6notes.htm
1 INTRODUCTION
At first the analysis of the very crowded emission spectrum rested on absorption data and on calculations which did not take into account the rotational
http://mer-du-sud.obspm.fr/intro.htm
Chapter 5
B. dark-line (absorption) spectrum. A. a continuous spectrum. B. emission lines only. C. absorption lines only. D. emission lines on a continuous spectrum.
http://www.astro.umn.edu/intro/syll/test5.html
Self absorption
The differential light intensity spectrum arriving at the PM photocathod is weighted by the emission spectrum and attenuated by its absorption.
http://www.fynu.ucl.ac.be/librairie/theses/luc.michel/these/node108.html
BD Biosciences : Pharmingen : Protocols
a superior fluorochrome for third color analysis because of its high emission intensity and broad spectrum. Because of its broad absorption range (Fig
http://www.bdbiosciences.com/pharmingen/protocols/Fluorochrome_Absorption.shtml
http://www.phy.davidson.edu/StuHome/BeDenius/rubidium/intro2.htm
The peaks in the spectrum occur at specific frequencies. Comparing the example absorption and emission spectra given here, one can see that the peaks occur
http://www.phy.davidson.edu/StuHome/BeDenius/rubidium/intro2.htm
LINESPEC: Create Spectra from Emission and/or Absorption Line Lists
61b. rvsao.linespec. linespec is an IRAF task in the rvsao package which creates a spectrum from a set of absorption or emission line positions. This spectrum is written into a one-dimensional
http://tdc-www.harvard.edu/iraf/rvsao/linespec/linespec.html
l12 Absorption and emission
The absorption line spectrum always appears, when atoms or molecules, which are not We will consider emission spectra below. Arc spectrum. Spark spectrum.
http://kr.cs.ait.ac.th/~radok/physics/l12.htm
XCSAO Example 2
After the command l (for lines) is typed, the spectrum is replotted with emission and absorption lines labelled at the velocity labelled by the asterisk (*).
http://tdc-www.harvard.edu/iraf/rvsao/xcsao/ex2/xcsao.ex2.html
AMASE Astronomical Object Attribute Hierarchy: Active Galaxy
2. (bandpass), 1. Featureless Nonthermal Spectrum. 2. Featureless (bandpass) Continuum Emission. 2. Line Emission. Line Absorption, Absorption.
http://amase.gsfc.nasa.gov/amase/amase_schema/actgal_attrib.html
Visible Spectrum - Student
the resulting spectrum is called a bright line emission spectrum. frequencies from white light, the spectrum produced is called an absorption spectrum.
http://fusioned.gat.com/Teachers/Curriculum/Curriculum-HTML/T01S-visible-light.html
Chapter 5 Answers
or smeared) emission and absorption lines is because: C. of the collisions between atoms causing doppler shifts 17) When we look at the continuous spectrum of
http://www.astro.umn.edu/intro/syll/test5.answers.html
Stellar Spectra
of continuum. an absorption spectrum or sometimes an absorption-line spectrum. an emission spectrum or emission-line spectrum. An
http://casswww.ucsd.edu/public/tutorial/Stars.html
More About Spectra and the Spectra of Galaxies
the visible portion of the spectrum), and because it is important to know the relative intensities and exact shape of of emission and absorption features (as
http://imagine.gsfc.nasa.gov/YBA/M31-velocity/spectra-more.html
The electronic structure of YBa Cu O studied by soft X-ray ...
Figure 2 shows the valence-core XES spectrum along with XAS spectrum. In the case of YBa 2 Cu 4 O 8 , the absorption-emission spectra show the unbroken density
http://alspubs.lbl.gov/AbstractManager/uploads/ACFD10.pdf
Atomic model for emission and absorption of radiation
Next: The continuous spectrum Up: Electromagnetic Radiation Previous: Characteristic wavelengths Contents Atomic model for emission and absorption of radiation.
http://www.phys.uri.edu/~chuck/ast108/notes/node28.html
The Bohr Atom: The Absorption Spectrum
emit. This yields a reasonable glucose absorption spectrum superimposed on the usual smooth blackbody emission spectrum. An approximate
http://www.control.co.kr/java1/masong/absorb.html
Scattering (and the blue sky)
as the hot solid object. The spectrum would look like: A continuous spectrum. An absorption spectrum. An emission spectrum. Emission and Absorption Spectra.
http://astron.berkeley.edu/~basri/astro10/Ppt/ISM&Galaxy.ppt
PIRA 7B11.00 ABSORPTION
emission, 39-1.9, A projection system is aligned so both emission and absorption lines of a second arc that vaporizes sodium and the spectrum produced shows
http://www.physics.ncsu.edu/pira/7modern/7B11.html
Lecture 3: Atoms and Spectra
a continuous black body spectrum; A hot, low-density gas produces an EMISSION spectrum; A cool, low-density gas produces an ABSORPTION spectrum; Every type of atom
http://www-astronomy.mps.ohio-state.edu/~ryden/ast162_1/notes3.html
Reminders Astronomy Picture of the Day More Spectra Emission ...
Absorption spectrum Intensity frequency Emission Lines Later is was discovered that if gases are heated until they emit light, a spectrum made up of bright
http://www.physics.ucla.edu/class/02F/3_Ghez/notes/reminderslec5.pdf
Emission spectrum
cb9. Next: Light yield Up: Measurement and results Previous: Absorption. Emission spectrum. During scintillator irradiation, new molecules could be created. These new molecules can modify the
http://www.fynu.ucl.ac.be/librairie/theses/luc.michel/these/node150.html
Bar-coding biomolecules with fluorescent nanocrystals
An 18 Å core absorbs and emits in the blue spectrum, whereas a 70 Å core emits in the red, and the absorption and emission wavelength are size-tunable in
http://www.nature.com/cgi-taf/DynaPage.taf?file=/nbt/journal/v19/n7/full/nbt0701_621.html
http://stingray.bio.cmu.edu/~web/sbio00/f3/f3.ps
Some distribution of dipoles will exist and this will lead to heterogeneous line broadening of both the absorption and emission spectrum of the fluorophore.
http://stingray.bio.cmu.edu/~web/sbio00/f3/f3.ps
OXYGEN ABSORPTION EDGE AND EMISSION LINES STRUCTURE.
Emission lines from all these elements are excited by an film produces an edge in the spectrum, in addition make a mesurement of the oxygen absorption edge of
http://acis.mit.edu/acis/spie96/gp_calpaper/node6.html
Developing and evaluating research-based classroom materials to ...
is absorbed when electrons [move to higher] energy states Q: Discuss the differences between the emission spectrum and the absorption spectrum: A: One
http://perlnet.umephy.maine.edu/research/spectro2000guelph.pdf
http://www.phy.davidson.edu/StuHome/BeDenius/rubidium/results.htm
There are four distinguishable peaks in the emission spectrum just as there are in the absorption spectrum. These four peaks fall
http://www.phy.davidson.edu/StuHome/BeDenius/rubidium/results.htm
Optical Properties of Color Stimuli
creating an emission spectrum. The light passes through some medium such as the atmosphere, or reflects off of some surface creating an absorption spectrum.
http://kiptron.psyc.virginia.edu/steve_boker/ColorVision2/node10.html
Reactive Species densities measured by optical emission and ...
in the plasma, using the Cl 2 absorption spectrum around 280 can be made : L off P on : Plasma emission (Lamp OFF Gas is ON L on P off : Lamp spectrum (Lamp ON
http://crppwww.epfl.ch/LTPD99/pdf/posters/neuilly.pdf
Board Questions: Electrons and Photons: Plus 2 Physics
in emission and absorption spectra.Find the wavelength of the spectral line which is present in the emission spectrum but absent in absorption spectrum.
http://www.plus2physics.com/electrons_and_photons/board_questions.asp?page=3
Spectral Lines in Stars - Absorbtion and Emission
For most elements, there is a certain temperature at which their emission and absorption lines are strongest. The lines you see in a stars spectrum act like
http://skyserver.fnal.gov/en/proj/advanced/spectraltypes/lines.asp
A Combined Diode Laser Absorption and Optical Emission ...
Infrared absorption spectrum of SiN radical around 2017cm^-1 and emission spectrum of SiCl_2, SiCl, Si, Cl, N_2 and N_2^+ at uv/visible region were detected.
http://www.eps.org/aps/meet/GEC02/baps/abs/S160007.html
The Bohr Atom
The highest energy series of the emission spectrum matches the absorption spectrum and is called the Lyman series. The emission
http://www.tannerm.com/bohratom.htm
RADIATIVE TRANSFER MODULES
Secondly, the absorption, emission, and reflection processes associated with the Earths clouds, and atmospheric aerosols attenuate the solar spectrum in very
http://www.arm.gov/docs/do(DELETED)ents/project/er_0441/bkground_5/over_radia_4.html
Background Information on Spectral Classification and the Color ...
Thus, one can think of the absorption spectrum to the right as the continuous spectrum minus the emission spectrum. Image Source: Arny Explorations Fig. 12.9,
http://physics.unl.edu/directory/lee/astroed/applets2/common/spectralclass.html
Spectroscopy … Study of the absorption, emission and scattering ...
Chemistry 306 Page 1 Spectroscopy ­ Study of the absorption, emission and scattering J s * = 1 calorie = 4.184 J The Electromagnetic Spectrum ­ Waves travel
http://www.rci.rutgers.edu/~layla/pharmchem/pdf_files/Spectroscopy.pdf
AMASE Astronomical Object Atribute Hierarchy: Spectral Attributes
(see Line Absorption for examples.). Children of Continuum Emission: Flat Spectrum, (bandpass), Flat (bandpass) Spectrum, 1. (bandpass) Continuum Emission.
http://amase.gsfc.nasa.gov/amase/amase_schema/spectral_attrib.html
Astronomy Notes
(Light). General properties of light, definition of frequency, spectrum, temperature. Light production: Continuous (thermal) spectra, emission lines, absorption lines and the Bohr model for the atom.
http://www.astronomynotes.com/
absorption line concept from the Astronomy knowledge base
Dark line in a spectrum, produced when light or other electromagnetic radiation coming from a distant source passes through a gas cloud or similar object closer to the observer. Like emission
http://www.site.uottawa.ca:4321/astronomy/absorptionline.html
Absorption spectrum
Energy Levels. Light Emission. Absorption Spectrum. Hydrogen-Like Ions. - Absorption Spectrum - Absorption Example Absorption Spectrum. Atoms can also absorb light as they emit it. Let?s send
http://library.thinkquest.org/16468/hydro-c1.htm
Fluorescent Highway Signs
Fluorescent Highway Signs. 5/18/00. Click here to start. Table of Contents. Title Page. Fluorescent Highway Signs: Main Topics. What is fluorescence? Absorption-Emission Spectrum. Bispectral
http://www.usd.edu/psyc301/nas/fluorence/index.htm
Time-resolved absorption and emission measurements of rotational ...
40 -30 -20 -10 0 10 20 30 40 % A bso rpti on Inten sity (ua .) Wavelength (nm) C 2 (1,1) C 2 (0,0) Absorption spectrum of C 2 Swan Band Emission spectrum of C
http://crppwww.epfl.ch/LTPD99/pdf/posters/duten.pdf
Emission line spectrum
the spectrum of IC 3639 similar to that of Mrk 477 (Heckman et al 1997). However, the absorption features are stronger in IC 3639 than in Mrk 477. The emission
http://www.iaa.es/~rosa/research/Seyferts/s2/node17.html
Spectrum of Quasar 0420-388 - Emission Lines
the principal emission line was estimated from the spectrum given in Wolstencroft et al. (1983). These authors also give the wavelengths of 15 absorption lines
http://www.achilles.net/~jtalbot/V1989/linedata.html
Lecture 10:Lecture 10: Atomic Physics for Kids of All Ages
Slide # 46: Absorption - step #2; electron spontaneous drops to lower energy state; emission; Emission is in a RANDOM direction; the continuous spectrum has dark
http://astro.gmu.edu/classes/a10594/notes/l10/l10.html
Further Explorations for Arnys Explorations, 2nd Ed.
What was most telling was that the dark lines in this absorption spectrum corresponded exactly to the bright lines in the emission spectrum if the same gas
http://www.mhhe.com/physsci/astronomy/arny/student/webtutor/Spectrum/
Annie Jump Cannon Homepage, understanding her work
the continuous spectrum, leaving dark absorption lines in there place, superimposed on the continuous spectrum. same wavelengths as the emission lines produced
http://www.wellesley.edu/Astronomy/annie/understanding.html
Emission and absorption lines
Emission and absorption lines. it is found to be made up of a series of ``lines, that is, the output from the prism is not a smooth spectrum of colors
http://phyun5.ucr.edu/~wudka/Physics7/Notes_www/node107.html
Quantum processes
Transitions between these quantized states occur by the photon processes absorption, emission, and stimulated emission. Electromagnetic spectrum. Index.
http://hyperphysics.phy-astr.gsu.edu/hbase/mod5.html
Light: An Introduction(Chap
Astronomical Spectra: What can we learn? In general, we see an underlying continuum spectrum with either or both absorption and emission features.
http://astrowww.astro.indiana.edu/~kai/a105/a105_5.doc
Effects of Radiative Emission and Absorption on the Propagation ...
for dry hydrocarbon-air mixtures, because of the differences in the absorption spectra of The second is that the emission spectrum Of C02 is broader at flame
http://microgravity.grc.nasa.gov/fcarchive/combustion/papers/Ju/Effects_of_Radiative.htm
GAUSS-Interactive fit of Gaussians to emission or absorption ...
QUIT - quit from program (spectrum analysis complete). Source comments: GAUSS Interactively fits Gaussians to an emission or absorption feature in a spectrum.
http://www.starlink.rl.ac.uk/star/docs/sun86.htx/node405.html
A cylindrical furnace for absorption spectral studies
Nostrand Reinhold) vol. 4 Lord Rayleigh 1927 Series of emission and absorption bands in the mercury spectrum. Proc. R. Soc. London A116
http://www.ias.ac.in/sadhana/Pdf2001Jun/Pe949.pdf
OPTICAL METHODS IN PROTEIN SCIENCE
FLUOROPHORES Page 31. FRET IS OBTAINED WHEN THE DONOR EMISSION SPECTRUM OVERLAPS WITH THE ACCEPTOR ABSORPTION SPECTRUM Page 32. FRET
http://www.dblab.helsinki.fi/~rtuma/protsci2002.pdf
AstroSoc - University of St Andrews Astronomical Society: ...
Absorption Emission Spectra Absorption and emission spectra are created when a hot gas is lit by a white light source (ie the entire EM spectrum).
http://www.st-andrews.ac.uk/~astrosoc/-astro/gloss-A.html
The HST-GHRS Spectrum of the Old Nova V603 Aql
and the emission center violet shifted by about 100 km s . In the case of the NV 1240Å doublet, the merged spectrum shows a blue-shifted absorption profile
http://www.stsci.edu/stsci/meetings/shst2/selvellip.html
Computation of the Output Absorption Spectrum
Next: Auxiliary Data Up: Typical Run Previous: Edition of the. Computation of the Output Absorption Spectrum. This is the main step achieved by the command: SYNEMI : input emission spectrum.
http://wwwsio.obspm.fr/sionline/doclib/midas/doc/94NOV/vol2/node203.html
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