The energy distribution in the visible spectrum for the 27 giants and supergiants of the M spectral type J/AZh/73/762 J/AZh/73/762 Energy distribution in giants and supergiants. The energy distribution in the visible spectrum for the 27 giants and supergiants of the M spectral type V M Tereshchenko Astron. Zh. 73 762 1996 1996AZh....73..762T Energy distributions Stars, giant giants supergiants energy distributions The energy distributions for 27 giants and supergiants of the M spectral type are presented in the region of 3200-7600{AA} with the step of 50{AA}. The observations were made in the Fessenkov Astrophysical institute (Alma-Ata) during 1986-1987 with a spectrophotometer of Seya-Namioka mounted on the 50-cm Cassegrain telescope. The primary standard is Vega with the energy distribution by Hayes (1985IAUS..111..225H). The relative r.m.s. of the results are given in the table3.dat.
Stars positions HD HD (Cat. <III/135>) name --- RAh Right ascension (2000) h RAm Right ascension (2000) min RAs Right ascension (2000) s DE- Declination sign --- DEd Declination (2000) deg DEm Declination (2000) arcmin DEs Declination (2000) arcsec Energy distribution lambda Spectral line wavelength 0.1nm HD36389 Energy distribution for HD 36389 10-8W/m2/cm HD42543 Energy distribution for HD 42543 10-8W/m2/cm HD44537 Energy distribution for HD 44537 10-8W/m2/cm HD78712 Energy distribution for HD 78712 10-8W/m2/cm HD206936 Energy distribution for HD 206936 10-8W/m2/cm HD1760 Energy distribution for HD 1760 10-8W/m2/cm HD19058 Energy distribution for HD 19058 10-8W/m2/cm HD20797 Energy distribution for HD 20797 10-8W/m2/cm HD23475 Energy distribution for HD 23475 10-8W/m2/cm HD197812 Energy distribution for HD 197812 10-8W/m2/cm HD224062 Energy distribution for HD 224062 10-8W/m2/cm HD18191 Energy distribution for HD 18191 10-8W/m2/cm HD18345 Energy distribution for HD 18345 10-8W/m2/cm HD55383 Energy distribution for HD 55383 10-8W/m2/cm HD55966 Energy distribution for HD 55966 10-8W/m2/cm HD56031 Energy distribution for HD 56031 10-8W/m2/cm HD69243 Energy distribution for HD 69243 10-8W/m2/cm HD77443 Energy distribution for HD 77443 10-8W/m2/cm HD80390 Energy distribution for HD 80390 10-8W/m2/cm HD84748 Energy distribution for HD 84748 10-8W/m2/cm HD123657 Energy distribution for HD 123657 10-8W/m2/cm HD132813 Energy distribution for HD 132813 10-8W/m2/cm HD184786 Energy distribution for HD 184786 10-8W/m2/cm HD196610 Energy distribution for HD 196610 10-8W/m2/cm HD202012 Energy distribution for HD 202012 10-8W/m2/cm HD222800 Energy distribution for HD 222800 10-8W/m2/cm HD224490 Energy distribution for HD 224490 10-8W/m2/cm Information about the stars Seq Running number --- HR Bright Star (Cat. <V/50>) number --- HD Henry Draper (Cat. <III/135>) number --- Names Other Names --- Vmag V magnitude mag B-V B-V color index mag U-B U-B color index mag Sptype Spectral type --- VarType Type of variability --- The observations and the accuracy of the results HD Henry Draper (Cat. <III/135>) number --- Dates Observation dates --- Std Standard star names --- Nobs Number of observations --- dM The difference of air masses dM is the difference of air masses of the program star and the standard star. --- dt The difference of time dt is the difference of time of the observations of the program star and the standard star min sigma1 rms in the range 3200-4000{AA} % sigma2 rms in the range 4000-5000{AA} % sigma3 rms in the range 5000-6000{AA} % sigma4 rms in the range 6000-7600{AA} % Veta Avedisova INASAN 1997Mar17 J_AZh_73_762.xml