The endpoint of the rp-process on accreting neutron stars

H. Schatz; A. Aprahamian; L. Bildsten; A. Cumming; M. Ouellette; T. Rauscher; Friedrich-Karl Thielemann; M. Wiescher

The endpoint of the rp-process on accreting neutron stars

H. Schatz, A. Aprahamian, L. Bildsten, A. Cumming, M. Ouellette, T. Rauscher, Friedrich-Karl Thielemann, M. Wiescher

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

Abstract

We find that the rp process in X-ray bursts and in steady state burning, for example in X-ray pulsars, ends in a SnSbTe cycle. We discuss the consequences for the neutron star crust composition an X-ray burst light curves.

Original language	English
Pages (from-to)	150C-153C
Number of pages	4
Journal	Nuclear Physics A
Volume	688
Issue number	1-2
Publication status	Published - 21 May 2001
Event	6th International Conference on Nuclei in the Cosmos - AARHUS, Denmark Duration: 27 Jun 2000 → 1 Jul 2000

Keywords

X-RAY-BURSTS

Cite this

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title = "The endpoint of the rp-process on accreting neutron stars",

abstract = "We find that the rp process in X-ray bursts and in steady state burning, for example in X-ray pulsars, ends in a SnSbTe cycle. We discuss the consequences for the neutron star crust composition an X-ray burst light curves.",

keywords = "X-RAY-BURSTS",

author = "H. Schatz and A. Aprahamian and L. Bildsten and A. Cumming and M. Ouellette and T. Rauscher and Friedrich-Karl Thielemann and M. Wiescher",

year = "2001",

month = may,

day = "21",

language = "English",

volume = "688",

pages = "150C--153C",

journal = "Nuclear Physics A",

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number = "1-2",

note = "6th International Conference on Nuclei in the Cosmos ; Conference date: 27-06-2000 Through 01-07-2000",

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TY - JOUR

T1 - The endpoint of the rp-process on accreting neutron stars

AU - Schatz, H.

AU - Aprahamian, A.

AU - Bildsten, L.

AU - Cumming, A.

AU - Ouellette, M.

AU - Rauscher, T.

AU - Thielemann, Friedrich-Karl

AU - Wiescher, M.

PY - 2001/5/21

Y1 - 2001/5/21

N2 - We find that the rp process in X-ray bursts and in steady state burning, for example in X-ray pulsars, ends in a SnSbTe cycle. We discuss the consequences for the neutron star crust composition an X-ray burst light curves.

AB - We find that the rp process in X-ray bursts and in steady state burning, for example in X-ray pulsars, ends in a SnSbTe cycle. We discuss the consequences for the neutron star crust composition an X-ray burst light curves.

KW - X-RAY-BURSTS

M3 - Article

SN - 0375-9474

VL - 688

SP - 150C-153C

JO - Nuclear Physics A

JF - Nuclear Physics A

IS - 1-2

T2 - 6th International Conference on Nuclei in the Cosmos

Y2 - 27 June 2000 through 1 July 2000

ER -

The endpoint of the rp-process on accreting neutron stars

Abstract

Keywords

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