Constraints on the number of X-ray Pulsars in IC 10 from a deep XMM-Newton Observation

Abstract

We report the most sensitive search yet for X-ray pulsars in the dwarf starburst galaxy IC 10, which is known to contain a population of young high mass X-ray binaries. We searched for pulsations in 207 point-like X-ray sources in the direction of IC 10 by a 2012 \xmm~observation with a total exposure time of 134.5 ks. Pulsation searches in faint objects can be sensitive to the energy bands of the light curves, and the source and background extraction areas. We analyzed separately the PN and MOS barycenter corrected 0.2-12 keV data, with good time interval filtering. Different schemes for source and background extraction were compared, and the search was repeated in the narrower 0.5-8 keV energy band to increase the signal-to-noise ratio. For the most conservative parameters, 5 point sources produced significant peaks in the Lomb-Scargle periodogram (99\% significance, single trial, assuming white noise). A similar number of different candidates result from alternative analyses. A $\sim$4100 s period seen in all 3 instruments for the black hole (BH) + Wolf-Rayet (WR) binary IC 10 X-1 is probably due to red noise of astrophysical origin. Considering the periods, luminosities, and spatial distribution of the pulsar candidates in the direction of IC 10, they do not belong to the same distribution as the ones in the Magellanic Clouds and Milky Way. This result holds even if the candidates are spurious, since if the Small Magellanic Cloud were placed at the distance of IC 10, we would expect to see $\sim$5 pulsars at $L_x>10^{36}$ \lx ~inside the $D_{25}$ contour, and their periods would be of order 100 seconds, rather than the mostly $\sim$1 s periods for the candidates reported here, which lie outside the main body of the galaxy.

6 pages, 1 figure

References in corpus (10)

• The Orbital Period of the Wolf-Rayet Binary IC 10 X-1; Dynamic Evidence that the Compact Object is a Black Hole
• Molecular Gas in the Low Metallicity, Star Forming Dwarf IC 10
• The Masses and Shapes of Dark Matter Halos from Galaxy-Galaxy Lensing in the CFHTLS
• A Long Look at the Be/X-Ray Binaries of the Small Magellanic Cloud
• The Chandra ACIS Timing Survey Project: glimpsing a sample of faint X-ray pulsators
• NGC300 X-1 and IC10 X-1: a new breed of black hole binary?
• A Transient Supergiant X-ray Binary in IC10. An Extragalactic SFXT?
• The X-ray Binary Population of the Nearby Dwarf Starburst Galaxy IC 10: Variable and Transient X-ray Sources
• A multi-observatory database of X-ray pulsars in the Magellanic Clouds
• Blue Supergiant X-ray Binaries in the Nearby Dwarf Galaxy IC 10

Cited by in corpus (1)

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