Effective temperature of B-type stars from the SI II lines of the UV multiplet 13.04 at 130.5-130.9 NM

Details Effective temperature of B-type stars from the SI II lines of the UV multiplet 13.04 at 130.5-130.9 NM Effective temperature of B-type stars from the SI II lines of the UV multiplet 13.04 at 130.5-130.9 NM

Jan 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...253..431s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 253, no. 2, Jan. 1992, p. 431-446.

Astronomy and Astrophysics

Astrophysics

8

B Stars, Line Spectra, Stellar Spectra, Stellar Temperature, Iue, Silicon

Scientific paper

An analysis was performed for the 129.3-132.0 nm region of ten normal and two helium-weak peculiar B-type stars of spectral types ranging from B2 to B9 and luminosity classes IV-V. Computations of spectra made it possible to determine the Si abundance from the Si III lines and to estimate the effective temperature from the Si III profiles. The rotational velocities of all the stars were also investigated.

Affiliated with

Also associated with

No associations

Rating

Effective temperature of B-type stars from the SI II lines of the UV multiplet 13.04 at 130.5-130.9 NM 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 Effective temperature of B-type stars from the SI II lines of the UV multiplet 13.04 at 130.5-130.9 NM, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Effective temperature of B-type stars from the SI II lines of the UV multiplet 13.04 at 130.5-130.9 NM will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-933572