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The discovery of an outburst and pulsed X-ray flux from SMC X-2 using the Rossi X-ray timing explorer

The discovery of an outburst and pulsed X-ray flux from SMC X-2 using the Rossi X-ray timing explorer
The discovery of an outburst and pulsed X-ray flux from SMC X-2 using the Rossi X-ray timing explorer
Rossi X-Ray Timing Explorer (RXTE) All-Sky Monitor observations of SMC X-2 show that the source experienced an outburst in 2000 January-April reaching a peak luminosity of greater than ~1038 ergs s-1. RXTE Proportional Counter Array observations during this outburst reveal the presence of pulsations with a 2.37 s period. However, optical photometry of the optical counterpart shows that the source was still significantly fainter than it was more than a half a year after the outburst in the 1970s when SMC X-2 was discovered.
Stars, Individual: Alphanumeric, SMC X-2, Neutron, X-Rays
0004-637X
L41-L44
Corbet, R.H.D.
04dfb23b-1456-46a3-9242-5cee983471d5
Marshall, F.D
222dc66e-1dac-48c8-81e8-0c84d91c897c
Coe, M.J.
a0a6390c-2109-492b-b94c-8993ffa962f4
Laycock, S.
3021ea8f-9d14-4cda-93cd-6776c37ed386
Handler, G
3dc6c09b-3bac-4f13-a8f8-aed4ea0c1614
Corbet, R.H.D.
04dfb23b-1456-46a3-9242-5cee983471d5
Marshall, F.D
222dc66e-1dac-48c8-81e8-0c84d91c897c
Coe, M.J.
a0a6390c-2109-492b-b94c-8993ffa962f4
Laycock, S.
3021ea8f-9d14-4cda-93cd-6776c37ed386
Handler, G
3dc6c09b-3bac-4f13-a8f8-aed4ea0c1614

Corbet, R.H.D., Marshall, F.D, Coe, M.J., Laycock, S. and Handler, G (2001) The discovery of an outburst and pulsed X-ray flux from SMC X-2 using the Rossi X-ray timing explorer. Astrophysical Journal, 548 (2), L41-L44. (doi:10.1086/318929).

Record type: Article

Abstract

Rossi X-Ray Timing Explorer (RXTE) All-Sky Monitor observations of SMC X-2 show that the source experienced an outburst in 2000 January-April reaching a peak luminosity of greater than ~1038 ergs s-1. RXTE Proportional Counter Array observations during this outburst reveal the presence of pulsations with a 2.37 s period. However, optical photometry of the optical counterpart shows that the source was still significantly fainter than it was more than a half a year after the outburst in the 1970s when SMC X-2 was discovered.

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More information

Submitted date: 25 September 2000
Published date: 10 February 2001
Keywords: Stars, Individual: Alphanumeric, SMC X-2, Neutron, X-Rays

Identifiers

Local EPrints ID: 37592
URI: http://eprints.soton.ac.uk/id/eprint/37592
ISSN: 0004-637X
PURE UUID: fd6e467f-71b3-4c69-a992-fc7ee5f97186
ORCID for R.H.D. Corbet: ORCID iD orcid.org/0000-0002-0763-8547

Catalogue record

Date deposited: 25 May 2006
Last modified: 16 Mar 2024 02:35

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Contributors

Author: R.H.D. Corbet ORCID iD
Author: F.D Marshall
Author: M.J. Coe
Author: S. Laycock
Author: G Handler

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