A dataset provided by the European Space Agency

Name: The candidate nebula of PSR J0855-4644 and the SE rim of SNR RX J0852.0-4622
Published: 2011-05-13T00:00:00Z

Proposal ID	060596
Title	The candidate nebula of PSR J0855-4644 and the SE rim of SNR RX J0852.0-4622
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0605960101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0605960201
DOI	https://doi.org/10.5270/esa-jon53gd
Principal Investigator, PI	Dr Fabio Acero
Abstract	The energetic pulsar J0855-4644 coincides with an enhancement in X-rays and TeVgamma-rays along the rim of the SNR RX J0852.0-4622, which could represent itspulsar wind nebula. We propose to study the spectrum and morphology of thiscandidate nebula to draw inferences about its nature, which cannot be doneconclusively with currently available X-ray data (from ASCA). We also propose tocharacterise the emission from the previously poorly studied South-East rim ofSNR RX J0852.0-4622. The wide field of view and broad energy coverage ofXMM-Newton will allow to disentangle these components from the foregroundthermal X-ray emission from the Vela SNR.
Publications	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 Discovery of a radio nebula around PSR J0855-4644 \|Maitra, C., Roy, S., et al. \| MNRAS \| 477-66 \| 2018 \| 2018MNRAS.477L..66M \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.477L..66M 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 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	2010-04-22T08:12:49Z/2010-04-23T01:30:06Z
Version	PPS_NOT_AVAILABLE
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	2011-05-13T00:00:00Z
Keywords	"broad energy coverage", "psr j0855 4644", "candidate nebula", "tev gamma rays", "xray data", "XMM", "south east rim", "draw inferences", "se rim", "vela supernova remnant", "J0852.0", "XMM-Newton", "pulsar wind nebula", "wide field", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Fabio Acero, 2011, 'The candidate nebula of PSR J0855-4644 and the SE rim of SNR RX J0852.0-4622', PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-jon53gd