Deepest far ultraviolet view of a central field in the Coma cluster by AstroSat UVIT

Deepest far ultraviolet view of a central field in the Coma cluster by AstroSat UVIT

We present analysis of the far ultraviolet (FUV) emission of sources in the central region of the Coma cluster (z=0.023) using the data taken by the UVIT aboard the multi-wavelength satellite mission AstroSat. We find a good correlation between the UVIT FUV flux and the fluxes in both wavebands of t...

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Veröffentlicht in:arXiv.org 2022-09
Hauptverfasser: Mahajan, Smriti, Kulinder Pal Singh, Postma, Joseph E, Pradeep, Kala G, Koshy, George, Côté, Patrick
Format: Artikel
Sprache:eng
Schlagworte:
Active galactic nuclei
Color
Emission analysis
Galactic clusters
Galaxies
Physics - Astrophysics of Galaxies
Quasars
Ram pressure
Star formation
Stars
Stars & galaxies
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Zusammenfassung:We present analysis of the far ultraviolet (FUV) emission of sources in the central region of the Coma cluster (z=0.023) using the data taken by the UVIT aboard the multi-wavelength satellite mission AstroSat. We find a good correlation between the UVIT FUV flux and the fluxes in both wavebands of the Galex mission, for the common sources. We detect stars and galaxies, amongst which the brightest (r
ISSN:2331-8422
DOI:10.48550/arxiv.2209.05886