Is Calvera a Gamma-ray Pulsar?
arXiv:1106.2140 · doi:10.1088/2041-8205/736/1/L3
Abstract
Originally selected as a neutron star (NS) candidate in the ROSAT All-Sky Survey, 1RXS J141256.0+792204 ("Calvera") was discovered to be a 59 ms X-ray pulsar in a pair of XMM-Newton observations (Zane et al. 2011). Surprisingly, their claimed detection of this pulsar in Fermi gamma-ray data requires no period derivative, severely restricting its dipole magnetic field strength, spin-down luminosity, and distance to small values. This implies that the cooling age of Calvera is much younger than its characteristic spin-down age. If so, it could be a mildly recycled pulsar, or the first "orphaned" central compact object (CCO). Here we show that the published Fermi ephemeris fails to align the pulse phases of the two X-ray observations with each other, which indicates that the Fermi detection is almost certainly spurious. Analysis of additional Fermi data also does not confirm the gamma-ray detection. This leaves the spin-down rate of Calvera less constrained, and its place among the families of NSs uncertain. It could still be either a normal pulsar, a mildly recycled pulsar, or an orphaned CCO.
5 pages, 4 figures, to appear in The Astrophysical Journal Letters
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Cited by in corpus (11)
- The Spin-down of PSR J0821-4300 and PSR J1210-5226: Confirmation of Central Compact Objects as Anti-Magnetars
- X-ray Measurement of the Spin-Down of Calvera: a Radio- and Gamma-ray-Quiet Pulsar
- Proper Motion and Timing of Two Unusual Pulsars: Calvera and 1E 1207.4-5209
- Neutron Star Interior Composition Explorer X-ray Timing of the Radio and Gamma-ray Quiet Pulsars PSR J1412+7922 AND PSR J1849-0001
- NICER study of pulsed thermal X-rays from Calvera: a neutron star born in the Galactic halo?
- The peculiar isolated neutron star in the Carina Nebula - Deep XMM-Newton and ESO-VLT observations of 2XMM J104608.7-594306
- Deep optical observations of unusual neutron star Calvera with the GTC
- The First Glitch in a Central Compact Object Pulsar: 1E 1207.4-5209
- Statistical ages and the cooling rate of X-ray dim isolated neutron stars
- Detection of the extended -ray emission from the high Galactic latitude Calvera's SNR candidate
- Calvera: A low-mass strangeon star torqued by debris disk?