Chandra Detection of the ``Duck'' Pulsar PSR B1757-24

Details Chandra Detection of the ``Duck'' Pulsar PSR B1757-24 Chandra Detection of the ``Duck'' Pulsar PSR B1757-24

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001tysc.confe..42k&link_type=abstract

Two Years of Science with Chandra, Abstracts from the Symposium held in Washington, DC, 5-7 September, 2001, meeting abstract.

Physics

Supernovae, Supernova Remnants And Isolated Neutron Stars

Scientific paper

We present Chandra/ACIS observations of the ``duck'' pulsar PSR B1757-24. In particular, we report the first X-ray detection of the point source, as well as the detection of faint extended emission in the direction of its radio trail. We discuss these results in the context of the pulsar's spin-down luminosity and its conversion into magnetospheric emission as well as the pulsar wind. In addition, we discuss constraints on the X-ray emission from the nearby supernova remnant G5.4-1.2.

Affiliated with

Also associated with

No associations

Rating

Chandra Detection of the ``Duck'' Pulsar PSR B1757-24 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Chandra Detection of the ``Duck'' Pulsar PSR B1757-24, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Chandra Detection of the ``Duck'' Pulsar PSR B1757-24 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1163304