GG Carinae: orbital parameters and accretion indicators from phase-resolved spectroscopy and photometry
B[ e ] supergiants are a rare and unusual class of massive and luminous stars, characterised by opaque circumstellar envelopes. GG Carinae is a binary whose primary component is a B[ e ] supergiant and whose variability has remained unsatisfactorily explained. Using photometric data from ASAS, OMC,...
| المؤلفون الرئيسيون: | , , , |
|---|---|
| التنسيق: | Journal article |
| اللغة: | English |
| منشور في: |
Oxford University Press
2020
|