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Near ultraviolet spectra of a group of early-type stars with Balmer emission

Journal Article:

Abstract

In the near ultraviolet region some absorption features in B stars are easily recognizable as criteria for assigning luminosity class. In the same region the characteristics displayed by Be stars suggest higher luminosities than in the photographic region. It appears that Fe II 2538-2548 A should be useful for studying the outer layers of stellar atmospheres.
Authors:
Ringuelet, A E [1] 
  1. Instituto de Astronomia y Fisica del Espacio, Buenos Aires (Argentina)
Publication Date:
Aug 01, 1980
Product Type:
Journal Article
Reference Number:
AIX-11-567548; EDB-81-101130
Resource Relation:
Journal Name: Mon. Not. R. Astron. Soc.; (United Kingdom); Journal Volume: 192:2
Subject:
71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; STARS; ULTRAVIOLET SPECTRA; ABSORPTION SPECTRA; BALMER LINES; IRON IONS; LUMINOSITY; NEAR ULTRAVIOLET RADIATION; STELLAR ATMOSPHERES; ATMOSPHERES; CHARGED PARTICLES; ELECTROMAGNETIC RADIATION; IONS; OPTICAL PROPERTIES; PHYSICAL PROPERTIES; RADIATIONS; SPECTRA; ULTRAVIOLET RADIATION; 640102* - Astrophysics & Cosmology- Stars & Quasi-Stellar, Radio & X-Ray Sources
OSTI ID:
6408945
Country of Origin:
United Kingdom
Language:
English
Other Identifying Numbers:
Journal ID: CODEN: MNRAA
Submitting Site:
INIS
Size:
Pages: 399-407
Announcement Date:

Journal Article:

Citation Formats

Ringuelet, A E. Near ultraviolet spectra of a group of early-type stars with Balmer emission. United Kingdom: N. p., 1980. Web.
Ringuelet, A E. Near ultraviolet spectra of a group of early-type stars with Balmer emission. United Kingdom.
Ringuelet, A E. 1980. "Near ultraviolet spectra of a group of early-type stars with Balmer emission." United Kingdom.
@misc{etde_6408945,
title = {Near ultraviolet spectra of a group of early-type stars with Balmer emission}
author = {Ringuelet, A E}
abstractNote = {In the near ultraviolet region some absorption features in B stars are easily recognizable as criteria for assigning luminosity class. In the same region the characteristics displayed by Be stars suggest higher luminosities than in the photographic region. It appears that Fe II 2538-2548 A should be useful for studying the outer layers of stellar atmospheres.}
journal = {Mon. Not. R. Astron. Soc.; (United Kingdom)}
volume = {192:2}
journal type = {AC}
place = {United Kingdom}
year = {1980}
month = {Aug}
}