MAXI/GSC detection of an increase in X-ray intensity from 4U 1630-47

Details MAXI/GSC detection of an increase in X-ray intensity from 4U 1630-47 MAXI/GSC detection of an increase in X-ray intensity from 4U 1630-47

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009atel.2363....1t&link_type=abstract

The Astronomer's Telegram, #2363

Astronomy and Astrophysics

Astronomy

2

X-Ray, Black Holes, Transients

Scientific paper

An increase of X-ray flux from the Galactic black hole candidate 4U1630-47 was detected by MAXI/GSC on 2009 December 29 (UT). The one-day averaged X-ray fluxes (1.5-20 keV) were about 9, 15, 21, and 38 mCrab for December 26,27,28, and 29 (UT) respectively. The MAXI/GSC light curves can be found at http://maxi.riken.jp/top/index.php?cid=000000000001&disp_mode=source . Please note that the fluxes of 4U1630-47 shown on the light curve web page are contaminated by the Galactic ridge emission, which has been subtracted in the fluxes reported above.

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