The transition to stable burning on an accreting neutron star

J. L. Fisker; W. Raphael Hix; M. Liebendörfer; F. K. Thielemann

doi:10.1016/S0375-9474(03)00902-3

The transition to stable burning on an accreting neutron star

J. L. Fisker, W. Raphael Hix, M. Liebendörfer, F. K. Thielemann

Research output: Contribution to journal › Article › peer-review

12 Scopus citations

Abstract

We describe the interplay between nucleosynthesis, convection, accretion, and the resulting composition on the surface of an accreting standard neutron star as a function of the accretion rate and find the dependence of the critical accretion rate on the core luminosity.

Original language	English
Pages (from-to)	614-616
Number of pages	3
Journal	Nuclear Physics A
Volume	723
Issue number	1-2
DOIs	https://doi.org/10.1016/S0375-9474(03)00902-3
State	Published - Jul 28 2003
Externally published	Yes

Funding

*supported by Swiss NSF grant 2000-061822

Funders	Funder number
Swiss NSF	2000-061822

Access to Document

10.1016/S0375-9474(03)00902-3

Cite this

@article{14758fabf87c4e3bae1b3f3b5db74456,

title = "The transition to stable burning on an accreting neutron star",

abstract = "We describe the interplay between nucleosynthesis, convection, accretion, and the resulting composition on the surface of an accreting standard neutron star as a function of the accretion rate and find the dependence of the critical accretion rate on the core luminosity.",

author = "Fisker, {J. L.} and Hix, {W. Raphael} and M. Liebend{\"o}rfer and Thielemann, {F. K.}",

year = "2003",

month = jul,

day = "28",

doi = "10.1016/S0375-9474(03)00902-3",

language = "English",

volume = "723",

pages = "614--616",

journal = "Nuclear Physics A",

issn = "0375-9474",

publisher = "Elsevier",

number = "1-2",

}

TY - JOUR

T1 - The transition to stable burning on an accreting neutron star

AU - Fisker, J. L.

AU - Hix, W. Raphael

AU - Liebendörfer, M.

AU - Thielemann, F. K.

PY - 2003/7/28

Y1 - 2003/7/28

N2 - We describe the interplay between nucleosynthesis, convection, accretion, and the resulting composition on the surface of an accreting standard neutron star as a function of the accretion rate and find the dependence of the critical accretion rate on the core luminosity.

AB - We describe the interplay between nucleosynthesis, convection, accretion, and the resulting composition on the surface of an accreting standard neutron star as a function of the accretion rate and find the dependence of the critical accretion rate on the core luminosity.

UR - http://www.scopus.com/inward/record.url?scp=0037572188&partnerID=8YFLogxK

U2 - 10.1016/S0375-9474(03)00902-3

DO - 10.1016/S0375-9474(03)00902-3

M3 - Article

AN - SCOPUS:0037572188

SN - 0375-9474

VL - 723

SP - 614

EP - 616

JO - Nuclear Physics A

JF - Nuclear Physics A

IS - 1-2

ER -

The transition to stable burning on an accreting neutron star

Abstract

Funding

Access to Document

Other files and links

Fingerprint

Cite this