Hot carbon stars - More about V348 SGR

Details Hot carbon stars - More about V348 SGR Hot carbon stars - More about V348 SGR

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987qjras..28..231h&link_type=abstract

Royal Astronomical Society, Quarterly Journal (ISSN 0035-8738), vol. 28, Sept. 1987, p. 231-238.

Astronomy and Astrophysics

Astronomy

4

Carbon Stars, Hot Stars, Peculiar Stars, Stellar Composition, Stellar Spectrophotometry, Variable Stars, Interstellar Extinction, Stellar Evolution, Stellar Models, Visible Spectrum

Scientific paper

New observational techniques (sensitive receivers, access to ultraviolet and infrared spectroscopy), as well as recent theoretical investigations on advanced stages of stellar evolution focus attention again on hydrogen-poor and helium-rich objects known as "carbon stars". The case of the hot peculiar variable V348 Sgr is discussed. New visible and infrared observations are presented, but the exact nature of the star remains much of an enigma.

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