4.7 Article

Hubble Space Telescope Nondetection of PSR J2144-3933: The Coldest Known Neutron Star

期刊

ASTROPHYSICAL JOURNAL
卷 874, 期 2, 页码 -

出版社

IOP Publishing Ltd
DOI: 10.3847/1538-4357/ab0f38

关键词

pulsars: individual (PSR J2144-3933); stars: neutron; ultraviolet: stars

资金

  1. NASA through a grant from the Space Telescope Science Institute [13783]
  2. NASA [NAS 5-26555]
  3. French Centre National d'Etudes Spatiales (CNES), of the ECOS-CONICYT program [C16U01]
  4. FONDECYT Post-doctoral Project [3150428]
  5. FONDECYT Regular Project [1150411]
  6. CONICYT project Basal [AFB-170002]

向作者/读者索取更多资源

We report nondetections of the similar to 3 x 10(8) yr old, slow, isolated, rotation-powered pulsar PSR J2144-3933 in observations with the Hubble Space Telescope in one optical band (F475X) and two far-ultraviolet bands (F125LP and F140LP), yielding upper bounds F-F475X < 22.7 nJy, F-F125LP < 5.9 nJy, and F-F140LP < 19.5 nJy, at the pivot wavelengths 4940 angstrom, 1438 angstrom and 1528 angstrom, respectively. Assuming a blackbody spectrum, we deduce a conservative upper bound on the surface (unredshifted) temperature of the pulsar of T < 42,000 K. This makes PSR J2144-3933 the coldest known neutron star, allowing us to study thermal evolution models of old neutron stars. This temperature is consistent with models with either direct or modified Urca reactions including rotochemical heating, and, considering frictional heating from the motion of neutron vortex lines, it puts an upper bound on the excess angular momentum in the neutron superfluid, J < 10(44) erg s.

作者

我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。

评论

主要评分

4.7
评分不足

次要评分

新颖性
-
重要性
-
科学严谨性
-
评价这篇论文

推荐

暂无数据
暂无数据