A dataset provided by the European Space Agency

Name 067162
Title Revealing the spin period of the isolated neutron star RX J1605.3+3249
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0671620101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0671620201

DOI 10.5270/esa-q63spk1
Author Dr Frank Haberl
Description From archival XMM-Newton data of the isolated neutron star RX J1605.3+3249 we found a candidate (2.5 sigma) period for the star.s rotation of 6.88 s. We propose a 56 ks observation to confirm this. The observation will also allow us to verify the existence of a narrow absorption line at 0.58 keV reported from the RGS spectrum (van Kerkwijk et al. 2004). If both, the suggested spin period and the narrow absorption line can be confirmed, RX J1605.3+3249 becomes a potential candidate among the ROSAT discovered isolated neutron stars with thermal X-ray spectrum to measure independently the mass and radius of the star. This would yield important constraints on the equation of state of matter in neutron stars.
Publication Unifying the observational diversity of isolated neutron stars via magneto-thermal evolution models . Vigano, D., Rea, N., et all. . MNRAS . 434-123 . 2013 . 2013MNRAS.434..123V ,
XMM-Newton reveals a candidate period for the spin of the "Magnificent Seven" neutron star RX J1605.3+3249 . Pires, A. M., Haberl, F., et all. . A&A . 563-50 . 2014 . 2014A&A...563A..50P ,
Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift . Yershov, V. N., . Ap&SS . 354-97 . 2014 . 2014Ap&SS.354...97Y ,
XMM-Newton publication statistics . Ness, J.-U., Parmar, A. N., et all. . AN . 335-210 . 2014 . 2014AN....335..210N ,
Ensemble X-ray variability of active galactic nuclei. II. Excess variance and updated structure function . Vagnetti, F., Middei, R., et all. . A&A . 593-55 . 2016 . 2016A&A...593A..55V ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Magnetic fields in neutron stars . Vigano, Daniele, . PhDT . 0-7 . 2013 . 2013PhDT.........7V ,
Narrow phase-dependent features in X-ray dim isolated neutron stars: a new detection and upper limits . Borghese, A., Rea, N., et all. . MNRAS . 468-2975 . 2017 . 2017MNRAS.468.2975B ,
A deep XMM-Newton look on the thermally emitting isolated neutron star RX J1605.3+...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2012-03-06T09:42:55Z/2012-03-07T03:52:28Z
Version 17.56_20190403_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations.
Since Earth's atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
Creator Contact https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published 2013-04-04T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013-04-04T00:00:00Z, 067162, 17.56_20190403_1200. https://doi.org/10.5270/esa-q63spk1