2002A&A...391.1033V

Query : 2002A&A...391.1033V

2002A&A...391.1033V - Astronomy and Astrophysics, volume 391, 1033-1037 (2002/9-1)

A review of X-ray spectral evolution in Crab pulsar.

VIVEKANAND M.

Abstract (from CDS):

Pravdo et al. (1997ApJ...491..808P) claimed that the phase resolved x-ray spectrum in Crab pulsar (PSR B0531+21) shows a spectral hardening at the leading edge of the first peak of its integrated profile (IP); this was a new and unexpected result. This article reanalyzes their data, as well as some other related data, and argues that the spectrum is as likely to be unvarying (i.e., neither hardening nor softening).

Abstract Copyright: ∼

Journal keyword(s): pulsars - individual: PSR B0531+21 - X-ray: stars - phase resolved spectra

Simbad objects: 3

Full paper

View the references in ADS

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 - 2023	#notes
1	M 1	SNR	05 34 30.9	+22 00 53						~	6059	1
2	V* CM Tau	Psr	05 34 31.9474694616	+22 00 52.153698024						~	5137	0
3	* alf CMi	SB*	07 39 18.11950	+05 13 29.9552	0.82	0.79	0.37	-0.05	-0.28	F5IV-V+DQZ	1847	0

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