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Optical spectroscopy and Doppler tomography of Cygnus X-2
P. Elebert
,
P. J. Callanan
, M. A.P. Torres
, M. R. Garcia
School of Physics
University College Cork
Harvard-Smithsonian Ctr. Astrophys.
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Dive into the research topics of 'Optical spectroscopy and Doppler tomography of Cygnus X-2'. Together they form a unique fingerprint.
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Physics
Tomography
100%
Circumstellar Disks
100%
Low-Mass X-Ray Binary Stars
100%
Gas Stream
100%
Radial-Velocity Method
66%
Neutron Stars
33%
Optical Identification
33%
Ephemeris
33%
X-Ray Bursts
33%
X Ray Irradiation
33%
Earth and Planetary Sciences
Emissions
100%
Tomography
100%
Accretion Disk
50%
Gas Stream
50%
X Ray Binaries
33%
Radial Velocity
33%
X Ray
16%
Ephemeris
16%
Neutron Stars
16%
X Ray Irradiation
16%
Immunology and Microbiology
X Ray
100%
Optical Spectroscopy
100%
Swan
100%
Face
25%
Engineering
Gas Stream
100%
Phase Present
33%
Radial Velocity Curve
33%