A dataset provided by the European Space Agency

Name: Period evolution of the remarkable CCO 1E 1207.4--5209
Published: 2010-01-30T00:00:00Z

Proposal ID	055281
Title	Period evolution of the remarkable CCO 1E 1207.4--5209
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0552810301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0552810401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0552810501
DOI	https://doi.org/10.5270/esa-gzj270c
Principal Investigator, PI	Dr George Pavlov
Abstract	1E 1207.4-5209, the central compact object in the SNR PKS 1209-51/52, showsabsorption lines in its thermal X-ray spectrum and 424 ms pulsations. Thephase-coherent timing of 14 XMM-Newton and Chandra observations of 2000-2005resulted in two timing solutions with different signs and very small magnitudesof period derivative. The spin-down solution suggests that 1E1207 is a neutronstar born with a rather low magnetic field and almost the same period as thatcurrently observed. The spin-up solution could be explained by a low-rateaccretion from a supernova debris disk. To find the unique timing solution andunderstand the properties of this enigmatic object, we propose new timingobservations, which will be phase-connected with all the previous observations.
Publications	On the Spin-down and Magnetic Field of the X-ray Pulsar 1E 1207.4-5209 \|Halpern J. P. Gotthelf E. V. \| ApJ \| 733-28 \| 2011 \| 2011ApJ...733L..28H \| http://ui.adsabs.harvard.edu/#abs/2011ApJ...733L..28H 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 \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch Eric W. \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F The Timing Behavior of the Central Compact Object Pulsar 1E 1207.4-5209 \|Gotthelf E. V. Halpern J. P. \| ApJ \| 900-159 \| 2020 \| 2020ApJ...900..159G \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...900..159G Classification of 4XMM-DR9 sources by machine learning \|Zhang Yanxia Zhao Yongheng \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII O VIII and Fe L-shell Transitions \|Pan Zeyang Qu Zhijie et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez Antonio C. \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R Robust constraints on feebly interacting particles using XMM-Newton \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2008-07-02T02:07:28Z/2008-12-22T18:20:52Z
Version	17.56_20190403_1200
Mission Description	The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs 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 Earths 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	2010-01-30T00:00:00Z
Last Update	2025-01-27
Keywords	"xmm newton", "supernova remnant", "enigmatic object", "phase coherent", "central compact object", "phase connected", "2000 2005 resulted", "cco 1e 1207", "absorption lines", "period evolution", "low magnetic field", "low rate accretion", "XMM-Newton", "thermal xray spectrum", "period derivative", "1e 1207", "424 ms pulsations", "XMM", "neutron star born", "supernova debris disk"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr George Pavlov, 2010, 'Period evolution of the remarkable CCO 1E 1207.4--5209', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-gzj270c