Publication Date:
2019-06-28
Description:
The ultraviolet energy distribution of the metal-poor supergiant HD 112374 is analyzed based on observations from the International Ultraviolet Explorer (IUE) satellite for the region between 1200 and 2000 A. A discontinuity was found in the UV spectra at 2600 A which confirmed the low-abundance of heavy elements found by Luck et al. (1983). Values for effective temperature and log g in HD112374 were consistent with the star being a very luminous Population II semi-regular variable. The full observational results are presented in a table.
Keywords:
ASTRONOMY
Type:
Astronomical Society of the Pacific, Publications (ISSN 0004-6280); 96; 897-902
Format:
text