Discovery of a 70.5 ms Pulsar in AX J1838.0-0655 Associated with HESS J1837-069

Details Discovery of a 70.5 ms Pulsar in AX J1838.0-0655 Associated with HESS J1837-069 Discovery of a 70.5 ms Pulsar in AX J1838.0-0655 Associated with HESS J1837-069

Feb 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atel.1392....1g&link_type=abstract

The Astronomer's Telegram, #1392

Astronomy and Astrophysics

Astronomy

1

Radio, X-Ray, >Gev, Neutron Stars, Pulsars, Supernova Remnants

Scientific paper

We have detected highly significant X-ray pulsations from the region of the TeV source HESS J1837-069 using the Rossi X-ray Timing Explorer (RXTE). The observatory was pointed at the steady X-ray source AX J1838.0-0655 (Bamba et al. 2003, ApJ, 589, 253) located within the HESS source, that has been conjectured to contain a pulsar wind nebula by Aharonian et al. 2006 (ApJ, 636, 777) and Malizia et al.

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