An ultraviolet spectral atlas of 10 Lacertae obtained with the Goddard high resolution spectrograph on the Hubble Space Telescope. J/AJ/116/941 J/AJ/116/941 10 Lac UV spectral atlas An ultraviolet spectral atlas of 10 Lacertae obtained with the Goddard high resolution spectrograph on the Hubble Space Telescope. J C Brandt S R Heap E A Beaver A Boggess K G Carpenter D C Ebbets J B Hutchings M Jura D S Leckrone J L Linsky S P Maran B D Savage A M Smith L M Trafton F M Walter R J Weymann M Snow T B Ake R H Hogen Astron. J. 116 941 1998 1998AJ....116..941B J/ApJS/93/211 : IUE survey of H I Ly{alpha} absorption. I. (Diplas+ 1994) Spectra, ultraviolet Stars, O atlases stars: early-type stars: individual (10 Lac) Observations of the narrow-lined O-type star 10 Lacertae taken with the Goddard High Resolution Spectrograph in 1992 November are presented. The spectra cover the wavelength range 1181-1777{AA} with a resolution of 15km/s and signal-to-noise ratio greater than 100:1. Absorption lines arising in the interstellar medium, the photosphere, and the stellar wind are identified and discussed.
HST HD 21468010 Lac22 39 15.7+39 03 01
 Interstellar absorption lines detected in the spectrum of 10 Lacertae LambLab Laboratory wavelength 0.1nm LamObs Observed Wavelength 0.1nm Species Species number=1 A single asterisk denotes an excited state, a double asterisk denotes a highly excited state --- HV Heliocentric velocity km/s Note Notes number=2 1: Line appears to be present, identified species is probably the dominant contributor to the observed absorption, blends are definite or likely. 2: Blend with C I {lambda}1188.883. 3: Line is definitely present, sharp and well resolved from neighboring lines; core is not saturated, no known or serious blends, wavelength and velocity appear consistent with other lines 4: Line is definitely present, core is saturated, wings are broader than unsaturated lines, wavelength and velocity appear consistent with other lines. 5: Saturated over 5{AA}. 6: Deep, nearly saturated. 7: Weak but real absorption feature is present at the expected wavelength. 8: Absorption is present in a complex stellar profile; photospheric or narrow absorption component contributions are possible. 9: Badly blended. -- Table of identified lines LamLab Laboratory wavelength 0.1nm LamObs Observed wavelength 0.1nm Com Comments --- James Marcout, Patricia Bauer CDS 1999Mar09 UNKNOWN UNKNOWN From AJ electronic version J_AJ_116_941.xml