PSR J1840–1419: A VERY COOL NEUTRON STAR
Creators
- 1. Max Planck Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn (Germany)
- 2. Department of Physics, West Virginia University, Morgantown, WV 26506 (United States)
- 3. University of Manchester, Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, Manchester M13 9PL (United Kingdom)
Description
We present upper limits on the X-ray emission for three neutron stars. For PSR J1840–1419, with a characteristic age of 16.5 Myr, we calculate a blackbody temperature upper limit (at 99% confidence) of kT ∞bb < 24+17–10 eV, making this one of the coolest neutron stars known. PSRs J1814–1744 and J1847–0130 are both high magnetic field pulsars, with inferred surface dipole magnetic field strengths of 5.5 × 1013 and 9.4 × 1013 G, respectively. Our temperature upper limits for these stars are kT ∞bb < 123+20–33 eV and kT ∞bb < 115+16–33 eV, showing that these high magnetic field pulsars are not significantly hotter than those with lower magnetic fields. Finally, we put these limits into context by summarizing all temperature measurements and limits for rotation-driven neutron stars.
Availability note (English)
Available from http://dx.doi.org/10.1088/0004-637X/764/2/180Additional details
Identifiers
Publishing Information
- Journal Title
- Astrophysical Journal
- Journal Volume
- 764
- Journal Issue
- 2
- Journal Page Range
- [4 p.]
- ISSN
- 0004-637X
- CODEN
- ASJOAB
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 44122155
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ASTRONOMY; ASTROPHYSICS; INTERSTELLAR MAGNETIC FIELDS; MAGNETIC DIPOLES; NEUTRON STARS; PHOTON EMISSION; PULSARS; ROTATION; TEMPERATURE MEASUREMENT
- Descriptors DEC
- COSMIC RADIO SOURCES; DIPOLES; EMISSION; MAGNETIC FIELDS; MOTION; MULTIPOLES; PHYSICS; STARS