Near-Infrared Observations of A0535+262

Details Near-Infrared Observations of A0535+262 Near-Infrared Observations of A0535+262

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.3020....1m&link_type=abstract

The Astronomer's Telegram, #3020

Astronomy and Astrophysics

Astronomy

1

Infra-Red, Optical, X-Ray, Binary, Transient, Pulsar

Scientific paper

Following the report of increase in the X-ray flux of the Be/X-ray binary pulsar A0535+262 since 2010 October 14 (Atel #2970), the photometric and spectroscopic observations were carried out in near-infrared J, H, and K-bands on 2010 October 28.9 UT and 31.9 UT using the 1.2 m Mt. Abu telescope operated by Physical Research Laboratory, Ahmedabad, India. The J, H, and K magnitudes of the Be star were estimated to be 7.69+/-0.02, 7.63+/-0.03 and 7.42+/-0.02 on 28 October 2010, and marginally brighter at 7.61+/-0.03, 7.50+/-0.02, and 7.40+/-0.02 on 31 October 2010 respectively.

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