2004ApJ...608L..61F


Query : 2004ApJ...608L..61F

2004ApJ...608L..61F - Astrophys. J., 608, L61-L64 (2004/June-2)

The nuclear reaction waiting points: 22Mg, 26Si, 30S, and 34Ar and bolometrically double-peaked type I X-ray bursts.

FISKER J.L., THIELEMANN F.-K. and WIESCHER M.

Abstract (from CDS):

Type I X-ray bursts with a double peak in the bolometric luminosity have been observed from several sources. The separation between the two peaks is on the order of a few seconds. We propose a nuclear waiting point impedance in the thermonuclear reaction flow to explain these observations. Nuclear structure information suggests the potential waiting points: 22Mg, 26Si, 30S, and 34Ar, which arise in conditions, where a further reaction flow has to await a β+-decay, because the (α,p)-reaction is too weak to overcome the target Coulomb barrier and the (p,γ)-reaction is quenched by photodisintegration at the burst temperature. The conclusion is that the effects of the experimentally unknown 30S(α,p)33Cl and 34Ar(α,p)37K might be directly visible in the observation of X-ray burst light curves.

Abstract Copyright: ∼

Journal keyword(s): Nuclear Reactions, Nucleosynthesis, Abundances - Stars: Neutron - X-Rays: Bursts

Simbad objects: 3

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Number of rows : 3
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 V* QX Nor LXB 16 12 43.0 -52 25 26           ~ 946 1
2 V* V801 Ara LXB 16 40 55.5976953528 -53 45 04.948107156 17.50 18.20 17.5   17.07 ~ 921 0
3 V* NP Ser LXB 18 16 01.7 -14 02 09   18.8       K 683 2

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