XMMSL1 J171900.4-353217 and XTE J1719-356 are Probably the Same Source

Details XMMSL1 J171900.4-353217 and XTE J1719-356 are Probably the Same Source XMMSL1 J171900.4-353217 and XTE J1719-356 are Probably the Same Source

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2615....1m&link_type=abstract

The Astronomer's Telegram, #2615

Astronomy and Astrophysics

Astronomy

X-Ray, Binaries, Black Holes, Neutron Stars, Pulsars, Transients

Scientific paper

Following the report of a new XMM slew transient, XMMSL1 J171900.4-353217 (Read & Saxton, ATEL #2607), we report the likely association to a transient designated XTE J1719-356, a faint transient source discovered in March 2010 by regular RXTE PCA monitoring observations of the galactic center. The monitoring observations detected enhanced emission from that region in March 2010. Follow-up dedicated PCA scanning and pointed observations 2010-03-10 detected a source.

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