A dataset provided by the European Space Agency

Name 074083
Title Trying Again to Complete a Study of the Brightest CCOs
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0740830201

DOI 10.5270/esa-2v71po9
Author Prof Jules Halpern
Description Central compact objects (CCOs) in supernova remnants (SNRs) represent a large fraction of neutron star births, but are difficult to study because of their weak magnetic fields. We have measured spin-down dipole fields for only three CCOs, of which two have spectral features that confirm their weak B-fields. In AO12, we proposed deep observations of the two remaining bright CCOs to search for their expected pulsations, and were given one A and one C target. Here we repropose the second target for AO13, and request a followup observation of the first target to confirm a possible period that was found in the AO12 observation. This program will establish the birth properties of an important class of NS, probe their magnetic field structure, and address pulsar evolution.
Publication Evidence for Thermal X-Ray Line Emission from the Synchrotron-dominated Supernova Remnant RX J1713.7-3946 . Katsuda, Satoru, Acero, Fabio, et all. . ApJ . 814-29 . 2015 . 2015ApJ...814...29K ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Spatially resolved spectroscopy of non-thermal X-rays in RX J1713.7-3946 with Chandra . Okuno, Tomoyuki, Tanaka, Takaaki, et all. . PASJ . 70-77 . 2018 . 2018PASJ...70...77O ,
X-ray observations of Galactic H.E.S.S. sources: An update . Puhlhofer, G., Eger, P., et all. . AN . 338-274 . 2017 . 2017AN....338..274P ,
Progressive steepening of the SNR RX J1713.7-3946 X-ray spectrum from XMM-Newton to INTEGRAL . Kuznetsova, Ekaterina, Krivonos, Roman, et all. . MNRAS . 489-1828 . 2019 . 2019MNRAS.489.1828K ,
Evolutionary Models for 43 Galactic Supernova Remnants with Distances and X-Ray Spectra . Leahy, D. A., Ranasinghe, S., . ApJS . 248-16 . 2020 . 2020ApJS..248...16L ,
Thermal luminosities of cooling neutron stars . Potekhin, A. Y., Zyuzin, D. A., et all. . MNRAS . 496-5052 . 2020 . 2020MNRAS.496.5052P ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2014-03-02T07:25:30Z/2014-03-03T22:32:10Z
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 2015-03-27T23:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2015-03-27T23:00:00Z, 074083, 17.56_20190403_1200. https://doi.org/10.5270/esa-2v71po9