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Helium ignition on accreting neutron stars with a new triple-α reaction rate

Peng, Fang and Ott, Christian D. (2010) Helium ignition on accreting neutron stars with a new triple-α reaction rate. Astrophysical Journal, 725 (1). pp. 309-312. ISSN 0004-637X. http://resolver.caltech.edu/CaltechAUTHORS:20110112-090206619

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Abstract

We investigate the effect of a new triple-α reaction rate from Ogata et al. on helium ignition conditions on accreting neutron stars and on the properties of the subsequent type I X-ray burst. We find that the new rate leads to significantly lower ignition column density for accreting neutron stars at low accretion rates. We compare the results of our ignition models for a pure helium accretor to observations of bursts in ultracompact X-ray binaries (UCXBs), which are believed to have nearly pure helium donors. For ^._m > 0.001 ^._m_(Edd), the new triple-α reaction rate from Ogata et al. predicts a maximum helium ignition column of ~3 × 10^9 g cm^(−2), corresponding to a burst energy of ~4 × 10^(40) erg. For ^._m ~ 0.01 ^._m_(Edd) at which intermediate long bursts occur, the predicted burst energies are at least a factor of 10 too low to explain the observed energies of such bursts in UCXBs. This finding adds to the doubts cast on the triple-α reaction rate of Ogata et al. by the low-mass stellar evolution results of Dotter & Paxton.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1088/0004-637X/725/1/309DOIUNSPECIFIED
http://iopscience.iop.org/0004-637X/725/1/309/PublisherUNSPECIFIED
Additional Information:© 2010 American Astronomical Society. Received 2010 August 19; accepted 2010 October 1; published 2010 November 17. It is a pleasure to thank Edward Brown for helpful comments which improved the paper. We thank Evan O’Connor, Hendrik Schatz and James Truran for useful discussions and comments. We thank the anonymous referee for helpful suggestions. We also thank Kazuyuki Ogata for providing us with his triple- α reaction rates. This work is partially supported through NSF grants AST-0855535 and OCI-0905046.
Group:TAPIR
Funders:
Funding AgencyGrant Number
NSFAST-0855535
NSFOCI-0905046
Subject Keywords:stars: neutron – X-rays: binaries – X-rays: bursts
Classification Code:PACS: 97.60.Jd; 97.10.Cv; 97.80.Jp; 97.10.Gz
Record Number:CaltechAUTHORS:20110112-090206619
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20110112-090206619
Official Citation:Fang Peng and Christian D. Ott 2010 ApJ 725 309 doi: 10.1088/0004-637X/725/1/309
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:21723
Collection:CaltechAUTHORS
Deposited By: Benjamin Perez
Deposited On:12 Jan 2011 19:25
Last Modified:26 Dec 2012 12:50

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