Program: GN-2012A-Q-67
Title: | The unique opportunity to determine the mass of an accreting neutron star: the eclipsing accretion powered X-ray pulsar SWIFT~J1749.4-2807 |
PI: | Peter Jonker |
Co-I(s): | Manuel Torres, Deepto Chakrabarty, Danny Steeghs |
Abstract
Last year it was discovered that the peculiar transient SWIFT J1749.4-2807
exhibits pulsations at 518 Hz. Furthermore, it turned out that the source was
eclipsing in a 8.8 hr orbit thereby holding the promise of a model independent
neutron star mass determination. Optical or near-infrared dynamical studies
offer the best prospects for constraining the neutron star equation of state, as
they do not rely on any specific models concerning the neutron star itself.
Unfortunately, the source position of SWIFT J1749.4-2807 is not well know at
present. The unique focusing capabilities of Chandra will provide the source position via our approved Chandra observation. Here, we propose for Gemini near-infrared imaging, to locate the near-infrared counterpart of the source. The time 0.2 hrs has been awarded via the Chandra TAC.
Publications using this program's data
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[data]
[ADS] Chandra X-ray and Gemini near-infrared observations of the eclipsing millisecond pulsar SWIFT J1749.4-2807 in quiescence