MODELING THE OPTICAL SPECTRUM OF ROMANO‘S STAR IN MINIMUM BRIGHTNESS
V532, known as Romano‘s star, is an interesting variable star located in the M33 galaxy. We study its spectral variability and the optical spectrum in minimum brightness. Using the non-LTE radiative transfer code CMFGEN we model the structure of its expanding atmosphere and stellar wind. The calcula...
| Main Authors: | , |
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| Format: | Article |
| Language: | English |
| Published: |
Odessa I. I. Mechnykov National University
2010-12-01
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| Series: | Odessa Astronomical Publications |
| Online Access: | http://oap.onu.edu.ua/article/view/85219 |