EVN detection of the newly-discovered black hole candidate MAXI J1836-194

Details EVN detection of the newly-discovered black hole candidate MAXI J1836-194 EVN detection of the newly-discovered black hole candidate MAXI J1836-194

Nov 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3790....1x&link_type=abstract

The Astronomer's Telegram, #3790

Astronomy and Astrophysics

Astronomy

Radio, Infra-Red, X-Ray, Binary, Black Hole, Transient

Scientific paper

The X-ray transient MAXI J1836-194 is most likely a Galactic stellar-mass black hole (ATel #3611, #3613, #3628, #3652) . It has been shown to harden in the X-rays and brighten in the infrared (ATel #3689). Here, we report on the detection of MAXI J1836-194 at 5 GHz with the European VLBI Network, in real-time e-VLBI observations on 2011 October 17. The transient source was detected with a flux density of 5.4 +- 0.3 mJy at RA 18h35m43.44555s, Dec.

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