A dataset provided by the European Space Agency

Name 067094
Title Revisiting the Pulsar Injection Problem
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670940101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670940201

DOI 10.5270/esa-anczg14
Author Dr Slavko Bogdanov
Description We propose XMM-Newton observations of three Galactic supernova remnants with positionally coincident radio pulsars in order to confirm or refute the plausible connection between the supposedly old (but possibly very young) pulsars and the supernova remnants. Based on this we could (i) constrain the Galactic population of neutron stars born spinning slowly, (ii) determine any connection between the new class of so-called anti-magnetars and normal radio pulsars, (iii) extend the grossly incomplete X-ray catalog of Galactic supernova remnants, and (iv) if the pulsars are not related to the remnants, look for a central compact object and-or a pulsar wind nebula.
Publication 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 ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Exploring the end states of massive stars using the X-ray emission of neutron stars and supernova remnants . Prinz, Tobias, . PhDT . 0-305 . 2013 . 2013PhDT.......305P ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2012-03-20T08:40:08Z/2012-03-20T14:29:52Z
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 2013-04-10T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013-04-10T00:00:00Z, 067094, 17.56_20190403_1200. https://doi.org/10.5270/esa-anczg14