EVLA observations suggest that M15 X-2 is the currently flaring source in M15

Details EVLA observations suggest that M15 X-2 is the currently flaring source in M15 EVLA observations suggest that M15 X-2 is the currently flaring source in M15

May 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3378....1m&link_type=abstract

The Astronomer's Telegram, #3378

Astronomy and Astrophysics

Astronomy

2

Radio, X-Ray, Binary, Globular Cluster, Neutron Star, Transient, Variables

Scientific paper

Following the detection of an X-ray flare in the globular cluster M15 (ATel #3356) and its subsequent Swift XRT localization to the cluster core (ATel #3363), we undertook EVLA observations to determine the source of the flaring event. The 1-hour observation on 2011 May 22 (12:11-13:11 UT) comprises of two 1024-MHz bands centred at 5.0 and 7.0 GHz. The array was in its BnA configuration, providing an angular resolution of 1.25 x 0.63 srq arcsec at 5 GHz and 0.92 x 0.50 sqr arcsec at 7 GHz.

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