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A Chandra Survey of the ‘Bar’ Region of the SMC

Published online by Cambridge University Press:  22 February 2018

A. Zezas ,
J. C. McDowell ,
P. Taylor ,
V. Kalogera ,
G. Fabbiano  and
D. Hadzidimitrion
A. Zezas
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden st., Cambridge;, MA 01238USA
J. C. McDowell
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden st., Cambridge;, MA 01238USA
P. Taylor
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden st., Cambridge;, MA 01238USA Boston College
V. Kalogera
Affiliation:
Northwestern University
G. Fabbiano
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden st., Cambridge;, MA 01238USA
D. Hadzidimitrion
Affiliation:
University of Crete, Greece

Extract

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We present the first results from a Chandra survey of the central region of the Small Magellanic Cloud. We detect a total of 122 sources down to a limiting luminosity of ~4.3 x 1033erg s–1, including 4 pulsars, 5 SNRs and two new transient sources. We also identify 18 more transient candidates based on comparison with ROSAT and ASCA surveys.

Type
The Contributed Papers
Information
International Astronomical Union Colloquium , Volume 194: Compact binaries in the galaxy and beyond , 2004 , pp. 205
Copyright
Copyright © Instituto de astronomia/revista mexicana de astronomίa y astrofίsica 2004

References

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