THE WHITE DWARF COMPANION OF A 2 M ☉ NEUTRON STAR
We report the optical discovery of the companion to the 2 M millisecond pulsar PSR J1614--2230. The optical colors show that the 0.5 M companion is a 2.2 Gyr old He-CO white dwarf. We infer that during the accretion phase is . We show that the pulsar was born with a spin close to its current value,...
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Veröffentlicht in: | Astrophysical journal. Letters 2011-08, Vol.737 (1), p.L1-jQuery1323916291473='48' |
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creator | Bhalerao, Varun B. Kulkarni, S. R. |
description | We report the optical discovery of the companion to the 2 M millisecond pulsar PSR J1614--2230. The optical colors show that the 0.5 M companion is a 2.2 Gyr old He-CO white dwarf. We infer that during the accretion phase is . We show that the pulsar was born with a spin close to its current value, well below the rebirth line. The spin-down parameters, the mass of the pulsar, and the age of the system challenge the simple recycling model for the formation of millisecond pulsars. |
doi_str_mv | 10.1088/2041-8205/737/1/L1 |
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Letters</title><description>We report the optical discovery of the companion to the 2 M millisecond pulsar PSR J1614--2230. The optical colors show that the 0.5 M companion is a 2.2 Gyr old He-CO white dwarf. We infer that during the accretion phase is . We show that the pulsar was born with a spin close to its current value, well below the rebirth line. 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R.</creator><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope><scope>OTOTI</scope></search><sort><creationdate>20110810</creationdate><title>THE WHITE DWARF COMPANION OF A 2 M ☉ NEUTRON STAR</title><author>Bhalerao, Varun B. ; Kulkarni, S. R.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c2661-51bed27246f50eca2730b0f436923c74d5e453b6d2ca3440d40464d048729e143</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2011</creationdate><topic>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</topic><topic>COSMIC RADIO SOURCES</topic><topic>DWARF STARS</topic><topic>NEUTRON STARS</topic><topic>PULSARS</topic><topic>STARS</topic><topic>WHITE DWARF STARS</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Bhalerao, Varun B.</creatorcontrib><creatorcontrib>Kulkarni, S. R.</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>OSTI.GOV</collection><jtitle>Astrophysical journal. Letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Bhalerao, Varun B.</au><au>Kulkarni, S. R.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>THE WHITE DWARF COMPANION OF A 2 M ☉ NEUTRON STAR</atitle><jtitle>Astrophysical journal. Letters</jtitle><date>2011-08-10</date><risdate>2011</risdate><volume>737</volume><issue>1</issue><spage>L1</spage><epage>jQuery1323916291473='48'</epage><pages>L1-jQuery1323916291473='48'</pages><issn>2041-8205</issn><eissn>2041-8213</eissn><abstract>We report the optical discovery of the companion to the 2 M millisecond pulsar PSR J1614--2230. The optical colors show that the 0.5 M companion is a 2.2 Gyr old He-CO white dwarf. We infer that during the accretion phase is . We show that the pulsar was born with a spin close to its current value, well below the rebirth line. The spin-down parameters, the mass of the pulsar, and the age of the system challenge the simple recycling model for the formation of millisecond pulsars.</abstract><cop>United States</cop><doi>10.1088/2041-8205/737/1/L1</doi><oa>free_for_read</oa></addata></record> |
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subjects | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY COSMIC RADIO SOURCES DWARF STARS NEUTRON STARS PULSARS STARS WHITE DWARF STARS |
title | THE WHITE DWARF COMPANION OF A 2 M ☉ NEUTRON STAR |
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