A dataset provided by the European Space Agency

Name: Search for the Outer Boundary of the Starburst Galaxy: NGC 253
Published: 2014-06-19T00:00:00Z

Proposal ID	072322
Title	Search for the Outer Boundary of the Starburst Galaxy: NGC 253
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0723220101
DOI	https://doi.org/10.5270/esa-b5n7iae
Principal Investigator, PI	Dr Mihoko Yukita
Abstract	We propose a 89 ks EPIC observation of the outskirts (out to 30 kpc from thecenter) of the nearby bright starburst galaxy, NGC 253. Our goal is to detectthe extended superwind emission at large radii. We will constrain the densityand temperature profiles of the wind emission and compare them with thetheoretical models. We will also search for extended clumpy features smilier tothe Northern Cap in M82. These data can place important constraints on howstarburst galaxies heat and enrich their environments.
Publications	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 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	2013-06-04T10:24:00Z/2013-06-05T16:48:30Z
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	2014-06-19T00:00:00Z
Keywords	"starburst galaxy", "M82", "temperature profiles", "superwind emission", "outer boundary", "ngc 253", "wind emission", "89 epic", "northern cap", "NGC 253", "EPIC", "starburst galaxy heat"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Mihoko Yukita, 2014, 'Search for the Outer Boundary of the Starburst Galaxy: NGC 253', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-b5n7iae