Discovery of two millisecond pulsars in Fermi sources with the Nancay Radio Telescope
Journal Article
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· The Astrophysical Journal
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- Observatoire de Paris, Nancay (France)
- Max-Planck-Institut fur Radioastronomie, Bonn (Germany)
- NASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States); Univ. of Maryland, College Park, MD (United States)
- Univ. Bordeaux, Gradignan (France)
- North-West Univ., Potchefstroom (South Africa)
- NASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States)
- Naval Research Lab., Washington, D.C. (United States)
- National Academy of Sciences, Washington, D.C. (United States); Naval Research Lab., Washington, D.C. (United States)
- Univ. of Maryland, College Park, MD (United States); NASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States)
- Univ. Paris Diderot, Gif sur Yvette (France)
- Columbia Univ., New York, NY (United States)
- Univ. of California, Berkeley, CA (United States)
- Australia Telescope National Facility, Epping, NSW (Australia)
- Max-Planck-Institut fur Radioastronomie, Bonn (Germany); The Univ. of Manchester (United Kingdom)
- The Univ. of Manchester (United Kingdom)
- Stanford Univ., Stanford, CA (United States)
- George Mason Univ., Fairfax, VA (United States); Naval Research Lab., Washington, D.C. (United States)
- National Radio Astronomy Observatory (NRAO), Charlottesville, VA (United States)
- Univ. of California, Santa Cruz, CA (United States)
Here, we report the discovery of two millisecond pulsars in a search for radio pulsations at the positions of Fermi-Large Area Telescope sources with no previously known counterparts, using the Nançay Radio Telescope. The two millisecond pulsars, PSRs J2017+0603 and J2302+4442, have rotational periods of 2.896 and 5.192 ms and are both in binary systems with low-eccentricity orbits and orbital periods of 2.2 and 125.9 days, respectively, suggesting long recycling processes. Gamma-ray pulsations were subsequently detected for both objects, indicating that they power the associated Fermi sources in which they were found. The gamma-ray light curves and spectral properties are similar to those of previously detected gamma-ray millisecond pulsars. Detailed modeling of the observed radio and gamma-ray light curves shows that the gamma-ray emission seems to originate at high altitudes in their magnetospheres. Additionally, X-ray observations revealed the presence of an X-ray source at the position of PSR J2302+4442, consistent with thermal emission from a neutron star. These discoveries along with the numerous detections of radio-loud millisecond pulsars in gamma rays suggest that many Fermi sources with no known counterpart could be unknown millisecond pulsars.
- Research Organization:
- SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
- Sponsoring Organization:
- USDOE
- Grant/Contract Number:
- AC02-76SF00515
- OSTI ID:
- 1357258
- Alternate ID(s):
- OSTI ID: 21574621
- Journal Information:
- The Astrophysical Journal, Journal Name: The Astrophysical Journal Journal Issue: 1 Vol. 732; ISSN 0004-637X
- Publisher:
- Institute of Physics (IOP)Copyright Statement
- Country of Publication:
- United States
- Language:
- English
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