2001A&A...380..516L


Query : 2001A&A...380..516L

2001A&A...380..516L - Astronomy and Astrophysics, volume 380516-519 (2001/12-3)

The gamma-ray source LSI +61deg303. I. RXTE/ASM observations.

LEAHY D.A.

Abstract (from CDS):

An analysis of RXTE/ASM observations of the unusual binary system LSI +61°303 is presented. The X-ray light curve gives a binary period of 26.42±0.05days, and an eccentricity of 0.30±0.04 (1σ). The eccentricity is determined by fitting an inverse Compton model to the X-ray light curve. These are the best determinations to date, as the optical period and eccentricity have larger uncertainties and published values of the radio period are variable. The radio outburst peak is not phase locked to the binary period, so the radio period is not the same as the binary period.

Abstract Copyright: ∼

Journal keyword(s): stars: neutron - stars: individual: LSI +61°303 - binaries: radio - stars: emission line, Be - stars X-rays:

Simbad objects: 2

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Number of rows : 2
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 LS I +61 303 HXB 02 40 31.6644419688 +61 13 45.593918580 11.27 11.61 10.75 10.19 9.55 B0Ve 903 2
2 ICRF J024457.6+622806 Sy1 02 44 57.6967097952 +62 28 06.517098084   12.15 12.19     ~ 310 2

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