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Examining the nature of the ultraluminous X-ray source Holmberg II X-1
F. Barra
, C. Pinto
, M. Middleton
, T. Di Salvo
,
D. J. Walton
, A. Gúrpide
, T. P. Roberts
Centre for Astrophysics Research (CAR)
Department of Physics, Astronomy and Mathematics
School of Physics, Engineering & Computer Science
Research output
:
Contribution to journal
›
Article
›
peer-review
10
Citations (Scopus)
20
Downloads (Pure)
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Keyphrases
XMM-Newton
100%
Ultraluminous X-ray Sources
100%
Publicly Available
50%
Thermal Component
50%
Thin Disk
25%
Accretion Flow
25%
GitHub
25%
Automated Scanning
25%
Spectral Coding
25%
Scientific Missions
25%
Nitrogen Compounds
25%
Stellar Clusters
25%
Emission Lines
25%
Accretion Rate
25%
Red Supergiants
25%
Bolometric Luminosity
25%
HTTPS
25%
Low Metallicity
25%
Stellar Mass Black Holes
25%
X-ray Spectra
25%
Eddington Limit
25%
Spectral Analysis
25%
Narrowband Emission
25%
High-resolution Spectra
25%
Broadband Spectrum
25%
Solar Abundances
25%
Compact Objects
25%
Science Archive
25%
High-resolution
25%
Power Law
25%
Rich Gas
25%
Accretion Discs
25%
Physics
X Ray Source
100%
High Resolution
100%
Spectrum Analysis
50%
X Ray Spectra
50%
Red Supergiant Stars
50%
Solar Abundances
50%
Metallicity
50%
Stellar Mass Black Holes
50%
Circumstellar Disks
50%
Compact Objects
50%
Earth and Planetary Sciences
European Space Agency
100%
X Ray Source
100%
Stellar Mass
33%
United States of America
33%
Power Law
33%
Spectrum Analysis
33%
Metallicity
33%
Emissions
33%
X Ray Spectra
33%