New millisecond pulsars from Fermi unidentified sources
Credit: NASA/DOE/Fermi LAT Collaboration; Paul Ray and the Fermi Pulsar Search Consortium

New Pulsars

There are objects whizzing through the Universe that we don't immediately recognize. The image above shows some of them - or at least it did. This image is the map of the Gamma-ray Universe obtained (and being obtained still) by the Fermi Gamma-ray Space Telescope. Fermi, as it's affectionately known (or FGRST, somewhat less affectionately) scans the sky and creates a new map of the entire Universe every few hours. It detects Gamma-ray emission from active galaxies (mostly), supernova remnants, starbursts; more than a 1000 objects so far. Many of the sources are mysterious, with no known counterparts at other wavelengths. Collaborations of astronomers are working hard to determine what these unknown sources are. The Fermi Pulsar Search Consortium is a group of radio astronomers dedicated to see if any of the detected Fermi sources are pulsars (neutron stars spinning rapidly in their graves) by looking for high frequency periodic signals from these GR sources. This effort has successfully shown that the 17 Fermi sources (circled above) are millisecond pulsars, extreme neutron stars rotating about 100 times or more per second. These strange, rare objects are old and have been spun up, probably by devouring a companion star over the course of a few billion years. Millisecond pulsars are precise natural clocks and are of special astrophysical interest. Continued study of these objects may lead to the discovery of another long-sought GR source: gravitational radiation.
Published: January 25, 2010

< HEA Dictionary * Archive * Search HEAPOW * Other Languages * HEAPOW on Facebook * Download all Images * Education >
Bookmark and Share

Each week the HEASARC brings you new, exciting and beautiful images from X-ray and Gamma ray astronomy. Check back each week and be sure to check out the HEAPOW archive!
Page Author: Dr. Michael F. Corcoran
Last modified Tuesday, 30-Mar-2010 11:17:21 EDT