On the spectrum of LDS 678B /EG 131/

Details On the spectrum of LDS 678B /EG 131/ On the spectrum of LDS 678B /EG 131/

Mar 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978mnras.182p..53w&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 182, Mar. 1978, p. 53P-56P.

Astronomy and Astrophysics

Astrophysics

4

Helium Hydrogen Atmospheres, Magnetic Stars, Stellar Spectra, White Dwarf Stars, Astrophysics, Continuous Spectra, Stellar Atmospheres

Scientific paper

Observations of the white dwarf LDS 678B obtained in 1976 show that it belongs to the helium-rich white-dwarf sequence. This finding indicates that the LDS 678B spectrum may have changed from a hydrogen-line to a continuous spectrum over the past 10 years. A lower limit of about 10,000 is deduced for the atmospheric helium to hydrogen ratio by number. The possibility that the star is a magnetic white dwarf is also discussed.

Affiliated with

Also associated with

No associations

Rating

On the spectrum of LDS 678B /EG 131/ does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with On the spectrum of LDS 678B /EG 131/, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the spectrum of LDS 678B /EG 131/ will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1082729