A dataset provided by the European Space Agency

Name: Probing magnetic field re-emergence through X-ray observations of radio pulsars
Published: 2019-02-26T23:00:00Z

Proposal ID	080424
Title	Probing magnetic field re-emergence through X-ray observations of radio pulsars
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0804240201
DOI	https://doi.org/10.5270/esa-qvqou77
Principal Investigator, PI	Mr Andrei Igoshev
Abstract	A significant fraction of young neutron stars can experience a strong fall-backepisode after a supernova explosion. The accreted matter screens the magneticfield which slowly diffuses out on a time scale of tens of thousand years whichis much shorter than the cooling timescale. However, no young radio pulsars withre-emerged magnetic field have been identified yet. The main goal of thisproposal is to detect for the first time the thermal emission from selected old(spin- down age more than 1 Myear) radio pulsars which allows us to confirm thefield re-emergence scenario.
Publications	Discovery of X-Rays from the Old and Faint Pulsar J1154--6250 \|Igoshev, Andrei P., Tsygankov, Sergey S., et al. \| ApJ \| 865-116 \| 2018 \| 2018ApJ...865..116I \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...865..116I 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 Charge Exchange X-Ray Emission Detected in Multiple Shells of Supernova Remnant G296.1-0.5 \|Tanaka, Yukiko, Uchida, Hiroyuki, et al. \| ApJ \| 933-101 \| 2022 \| 2022ApJ...933..101T \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...933..101T 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
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2018-02-08T01:11:59Z/2018-02-08T18:10:02Z
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	2019-02-26T23:00:00Z
Keywords	"magnetic field", "accreted matter screens", "neutron stars", "cooling timescale", "time scale", "supernova explosion", "thermal emission", "myear radio pulsars", "slowly diffuses", "radio pulsars"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Mr Andrei Igoshev, 2019, 'Probing magnetic field re-emergence through X-ray observations of radio pulsars', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-qvqou77