GG Carinae: Discovery of orbital phase dependent 1.583-day periodicities in the B[e] supergiant binary
GG Carinae (GG Car) is a binary whose primary component is a B[e] supergiant. Using photometric data from the Transiting Exoplanet Survey Satellite (TESS), All Sky Automated Survey (ASAS), Optical Monitoring Camera (OMC), and All Sky Automated Survey for Supernovae (ASAS-SN), and spectroscopic data...
Main Authors: | Porter, A, Blundell, K, Podsiadlowski, P, lee, S |
---|---|
格式: | Journal article |
語言: | English |
出版: |
Oxford University Press
2021
|
相似書籍
-
GG Carinae: orbital parameters and accretion indicators from phase-resolved spectroscopy and photometry
由: Porter, A, et al.
出版: (2020) -
GG Carinae: Orbital parameters and accretion indicators from phase-resolved spectroscopy and photometry
由: Porter, A, et al.
出版: (2020) -
THE PROGENITOR OF SUPERNOVA-1993J - A STRIPPED SUPERGIANT IN A BINARY-SYSTEM
由: Podsiadlowski, P, et al.
出版: (1993) -
Classical Nova Carinae 2018: Discovery of circumbinary iron and oxygen
由: McLoughlin, D, et al.
出版: (2020) -
Accretion in supergiant High Mass X-ray Binaries
由: Manousakis Antonios, et al.
出版: (2014-01-01)