The Nitrogen Abundance in Be Stars Determined from UV Spectra

Details The Nitrogen Abundance in Be Stars Determined from UV Spectra The Nitrogen Abundance in Be Stars Determined from UV Spectra

Jul 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..272..101p&link_type=abstract

Active OB stars: structure, evolution, mass loss, and critical limits, Proceedings of the International Astronomical Union, IAU

Astronomy and Astrophysics

Astronomy

1

Stars: Abundances, Stars: Emission-Line, Be, Stars: Rotation, Stars: Evolution

Scientific paper

A NLTE abundance analysis of the IUE spectra of 8 Be stars with v sin i
< 150km s-1 reveals no evidence for nitrogen enrichment
from mixing of core and photospheric material.

Affiliated with

Also associated with

No associations

Rating

The Nitrogen Abundance in Be Stars Determined from UV Spectra 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 The Nitrogen Abundance in Be Stars Determined from UV Spectra, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Nitrogen Abundance in Be Stars Determined from UV Spectra will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-995151