A dataset provided by the European Space Agency

Name 010926
Title LH9 and LH10: two LMC OB associations of different ages in one shot
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0109260101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0109260201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0109260301

DOI 10.5270/esa-uym4qq8
Author Prof Keith Mason
Description GT- Wang & Helfand (1991) reported the detection of diffuse X-ray emission from OB associations in the LMC with the Einstein observatory. Most of these associations are surrounded by H alpha rings or complex filaments, some of them, the so-called supergiant shells, extending over up to 1 kpc. Several of the associations exhibit shell-like X-ray morphologies which generally follow the H alpha emitting gas. According to the authors a significant part of the energy is provided by supernova remnants hitting the dense shells of young bubbles. This proposal is part of a comprehensive program aimed at the study of stars in different evolutionary stages and in environments with differeent metallicities.
Publication XMM-Newton observations of the giant H II region N 11 in the LMC . Naze, Y., Antokhin, I. I., et all. . A&A . 418-841 . 2004 . 2004A&A...418..841N ,
Searching for Diffuse Nonthermal X-Rays from the Superbubbles N11 and N51D in the Large Magellanic Cloud . Yamaguchi, H., Sawada, M., . ApJ . 715-412 . 2010 . 2010ApJ...715..412Y ,
The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue . Watson, M. G., Schroder, A. C., et all. . A&A . 493-339 . 2009 . 2009A&A...493..339W ,
Quasi-stellar Object Selection Algorithm Using Time Variability and Machine Learning: Selection of 1620 Quasi-stellar Object Candidates from MACHO Large Magellanic Cloud Database . Kim, Dae-Won, Protopapas, Pavlos, et all. . ApJ . 735-68 . 2011 . 2011ApJ...735...68K ,
Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras . Mateos, S., Saxton, R. D., et all. . A&A . 496-879 . 2009 . 2009A&A...496..879M ,
A Refined QSO Selection Method Using Diagnostics Tests: 663 QSO Candidates in the Large Magellanic Cloud . Kim, Dae-Won, Protopapas, Pavlos, et all. . ApJ . 747-107 . 2012 . 2012ApJ...747..107K ,
The XMM Cluster Survey: optical analysis methodology and the first data release . Mehrtens, Nicola, Romer, A. Kathy, et all. . MNRAS . 423-1024 . 2012 . 2012MNRAS.423.1024M ,
XMM-Newton data processing for faint diffuse emission. Proton fl...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2001-04-16T22:59:45Z/2001-09-17T11:03:13Z
Version PPS_NOT_AVAILABLE
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 2002-10-23T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2002-10-23T00:00:00Z, 010926, PPS_NOT_AVAILABLE. https://doi.org/10.5270/esa-uym4qq8