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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 =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:
FileName Lrecl Records Explanations
ReadMe 80 . This file stars.dat 114 16 Main photometry and spectral characteristics table3.dat 100 88 Energy distributions of S and carbon stars
Byte-by-byte Description of file: stars.dat
Bytes Format Units Label Explanations
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
Byte-by-byte Description of file: table3.dat
Bytes Format Units Label Explanations
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)
Note (1): 10nW/m2/cm=10-5.erg/(cm2.s.cm)

(End) Veta Avedisova [INASAN] 31-Jul-2000
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