The RXTE/ASM reveals rebrightening of GROJ1655-40

Details The RXTE/ASM reveals rebrightening of GROJ1655-40 The RXTE/ASM reveals rebrightening of GROJ1655-40

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005atel..445....1s&link_type=abstract

The Astronomer's Telegram, #445

Astronomy and Astrophysics

Astronomy

1

Optical, X-Ray, Binaries, Black Holes, Transients

Scientific paper

The RXTE/ASM reveals rebrightening of GROJ1655-40. The 1-day averaged x-ray intensity of GRO J1655-40 has been declining since its maximum of 1.70±0.02 Crab (2-12 keV) on 2005 Mar 19 (UT), reaching a minimum of 940±10 mCrab on Mar 26. On Mar 27, the average intensity was 960±10 mCrab. The average of the five 90-s observations taken on Mar 28 (at this writing) yield an average of 1.06±0.03 Crab, indicating that the source is rebrightening or possibly undergoing short-term flaring.

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