J/AZh/76/604 Spectrophotometry of S and carbon stars (Tereshchenko, 1999)
Spectrophotometry of three S stars and thirteen carbon N stars.
Tereshchenko V.M.
<Astron. Zh. 76, 604 (1999)>
=1999AZh....76..604T 1999AZh....76..604T
=1999ARep...43..526T 1999ARep...43..526T
ADC_Keywords: Stars, carbon ; Stars, S ; Energy distributions
Description:
The absolute energy distributions in the visual spectra
(3200-7600Å) of 13 N carbon stars and three S stars have been
investigated. The spectral resolution of the data is 50 A and the
relative rms error is 2-5%. The data supplement and extend the Almaty
and other spectrophotometric catalogs that are lacking in these types
of objects.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
stars.dat 114 16 Main photometry and spectral characteristics
table3.dat 100 88 Energy distributions of S and carbon stars
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Byte-by-byte Description of file: stars.dat
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Bytes Format Units Label Explanations
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1 A1 --- Type [CS] C: carbon star, S: S star
3- 4 I2 h RAh Right ascension (J2000.0)
6- 7 I2 min RAm Right ascension (J2000.0)
9- 12 F4.1 s RAs Right ascension (J2000.0)
14 A1 --- DE- Declination sign (J2000.0)
15- 16 I2 deg DEd Declination (J2000.0)
18- 19 I2 arcmin DEm Declination (J2000.0)
21- 22 I2 arcsec DEs Declination (J2000.0)
25- 28 I4 --- HR HR (Cat. V/50) number
31- 36 I6 --- HD HD (Cat. III/135) number
38- 48 A11 --- Name Star Name
50- 53 F4.2 mag Vmag V magnitude
55- 58 F4.2 mag B-V B-V colour index
60- 63 F4.2 mag U-B ? U-B colour index
65- 68 A4 --- SpType Spectral type
70- 72 A3 --- VarType Type of variability
74-114 A41 --- Obs Observation dates
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Byte-by-byte Description of file: table3.dat
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Bytes Format Units Label Explanations
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1- 4 I4 0.1nm lambda Spectral line wavelength
7- 10 I4 10nW/m2/cm BDCam Energy distribution for BD Cam (1)
13- 16 I4 10nW/m2/cm omiOri Energy distribution for omicron Ori (1)
19- 22 I4 10nW/m2/cm chiCyg Energy distribution for chi Cyg (1)
25- 28 I4 10nW/m2/cm RLep Energy distribution for R Lep (1)
31- 34 I4 10nW/m2/cm WOri ? Energy distribution for W Ori (1)
37- 40 I4 10nW/m2/cm YTau Energy distribution for Y Tau (1)
43- 46 I4 10nW/m2/cm BLOri Energy distribution for BL Ori (1)
49- 52 I4 10nW/m2/cm UUAur Energy distribution for UU Aur (1)
55- 58 I4 10nW/m2/cm XCnc Energy distribution for X Cnc (1)
61- 64 I4 10nW/m2/cm UHya Energy distribution for U Hya (1)
67- 70 I4 10nW/m2/cm VYUMa Energy distribution for VY UMa (1)
73- 76 I4 10nW/m2/cm YCVn Energy distribution for Y CVn (1)
79- 82 I4 10nW/m2/cm SSct ? Energy distribution for S Sct (1)
85- 88 I4 10nW/m2/cm VAql Energy distribution for V Aql (1)
91- 94 I4 10nW/m2/cm v460Cyg Energy distribution for v460 Cyg (1)
97-100 I4 10nW/m2/cm 19Psc Energy distribution for 19 Psc (1)
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Note (1): 10nW/m2/cm=10-5.erg/(cm2.s.cm)
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(End) Veta Avedisova [INASAN] 31-Jul-2000