Spectral synthesis for Be stars

Details Spectral synthesis for Be stars Spectral synthesis for Be stars

Jul 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..272..426s&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: Emission-Line, Be, Circumstellar Matter, Radiative Transfer

Scientific paper

A new monochromatic imaging and spectral synthesis package for Be stars,
based on the bedisk code, is introduced. Example images and spectra are
given for for H i and Fe ii. Predicted Fe ii equivalents widths are also
compared to recent observations by Arias et al. (2006) and show good
agreement, although only for very dense disks.

Affiliated with

Also associated with

No associations

Rating

Spectral synthesis for Be stars 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 Spectral synthesis for Be stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectral synthesis for Be stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-995565