Discovery of a strong emission line at 0.5 keV in MAXI J0556-332 with the RGS on XMM-Newton

Details Discovery of a strong emission line at 0.5 keV in MAXI J0556-332 with the RGS on XMM-Newton Discovery of a strong emission line at 0.5 keV in MAXI J0556-332 with the RGS on XMM-Newton

May 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3349....1m&link_type=abstract

The Astronomer's Telegram, #3349

Astronomy and Astrophysics

Astronomy

1

X-Ray, Binary, Transient

Scientific paper

MAXI J0556-332 was observed twice during its ongoing outburst (see,
e.g., ATEL #3102, #3103, #3104, #3106, #3110, #3112, #3116, #3119,
#3327) with ESA's XMM-Newton observatory, triggered as
target-of-opportunity (ToO) observations.

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