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VI/50 Energy Dist Stellar Spectra. V. Normal Stars (Sviderskiene 1988)
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Energy Distribution in the Stellar Spectra of Different Spectral Types and
Luminosities. V. Normal Stars
Sviderskiene Z.
<Vilniaus Astron. Obs. Biul. No. 80 (1988)>
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ADC_Keywords: Energy distributions ; Spectrophotometry
Description:
Mean energy distributions are given for 98 normal stars in the spectral
range from O to M and luminosity classes I, II, III, IV, and V. The
points cover the wavelength range from 1200A to 10500A and a include a
point at 12500A.
Introduction:
The energy distributions were based on photometric and
spectrophotometric data from many authors. All stars are dereddened. The
zero point for each wavelength is based on a Vega model atmosphere by
Mihalas (1966) with theta effective = 0.525 and log G = 4. It has been
extended into the ultraviolet using the OAO 2 results. This energy
distribution is given in the first file and can be used to change to
another system if desired. The ultraviolet portions are based on the IUE
calibrations. The energy distributions are given in intensities per unit
wavelength interval normalized to 100 at 5500A. Each value given in the
catalog is the intensity in the interval delta lambda = 50A centered on
the given wavelength.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
doc_01 80 124 desc
data_01.dat 80 3304 data
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Byte-by-byte Description of file: data_01.dat
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Bytes Format Units Label Explanations
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1- n In --- --- ---
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(End) Gail L. Schneider [SSDOO/ADC] 25-Sep-1995