Swift X-ray observations of classical novae. II. Virtual Observatory Resource

Authors

1. Schwarz G.J.
2. Ness J.-U.
3. Osborne J.P.
4. Page K.L.
5. Evans P.A.,Beardmore A.P.
6. Walter F.M.
7. Helton L.A.
8. Woodward C.E.
9. Bode M.,Starrfield S.
10. Drake J.J.

Published by

CDS

Abstract

The Swift gamma-ray burst satellite is an excellent facility for studying novae. Its rapid response time and sensitive X-ray detector provides an unparalleled opportunity to investigate the previously poorly sampled evolution of novae in the X-ray regime. This paper presents Swift observations of 52 Galactic/Magellanic Cloud novae. We included the X-Ray Telescope (0.3-10keV) instrument count rates and the UltraViolet and Optical Telescope (1700-8000{AA}) filter photometry. Also included in the analysis are the publicly available pointed observations of 10 additional novae the X-ray archives. This is the largest X-ray sample of Galactic/Magellanic Cloud novae yet assembled and consists of 26 novae with Super Soft X-ray emission, 19 from Swift observations.

Keywords

1. novae
2. x-ray-sources
3. photometry

Bibliographic source Bibcode

2011ApJS..197...31S

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https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/197/31

IVOA Identifier IVOID

ivo://CDS.VizieR/J/ApJS/197/31

Document Object Identifer DOI

doi:10.26093/cds/vizier.21970031

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