Abstract
On November 1st. RXTE-PCA scans of the Aql region detected X-ray
emission consistent with the neutron star transient and atoll source Aql
X-1. Further scans and pointed PCA observations show a rising X-ray
flux; the most recent flux is about 40 mCrab. Swift observed the
field for about 2.5 ksec on November 8th, 2009, and detected a bright
X-ray source at a position consistent with Aql X-1.
Original language | English (US) |
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Journal | The Astronomer's Telegram |
Volume | 2288 |
State | Published - Nov 1 2009 |
Keywords
- Request for Observations
- Binaries
- Neutron Stars
- Transients