Outburst from EXO 2030+375

Details Outburst from EXO 2030+375 Outburst from EXO 2030+375

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006atel..843....1c&link_type=abstract

The Astronomer's Telegram, #843

Astronomy and Astrophysics

Astronomy

8

X-Ray, Binaries, Neutron Stars, Transients

Scientific paper

Observations with the RXTE All-Sky Monitor of the Be/neutron star binary EXO 2030+375 reveal a recent increase in flux that indicates a change of source state. EXO 2030+375 has been seen with the ASM to exhibit regular outbursts on the known 46 day orbital period since the start of observations over 10 years ago on MJD 50087. The mean flux at orbital maximum is 1.6 counts/s in the 1.5 to 12 keV range (~20 mCrab) for the entire mission light curve, and larger peak fluxes of approximately 4 counts/s (~50 mCrab) have been detected during the last few years (e.g.

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