Published February 20, 2013 | Version v1
Journal article

PSR J1840–1419: A VERY COOL NEUTRON STAR

  • 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/764/2/180

Additional 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