A dataset provided by the European Space Agency

Name 006174
Title A1367 -- A Cluster in Formation
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0061740101

DOI 10.5270/esa-h1vgpom
Author Dr William Forman
Description Abell 1367 is an X-ray bright, nearby cluster containing an unusual set of small arc minute size clumps. Of the 16 clumps detected in Einstein and ROSAT observations, only 9 are associated with galaxies. Recent numerical simulations suggest that dense dark halos, formed at early epochs, can survive the cluster tidal field and halo-halo interactions. Perhaps the observed clumps are relics of these dense halos. We propose a 30ksec XMM observation that will cover the central region of the cluster and provide sufficient data to (1) accurately measure the spectra of individual clumps, (2) provide an accurate temperature map of the cluster on scales as small as 1 arc minute, and (3) for the brighter clumps, provide a spatially resolved temperature profile that will be used to
Publication HIFLUGCS: Galaxy cluster scaling relations between X-ray luminosity, gas mass, cluster radius, and velocity dispersion . Zhang, Y.-Y., Andernach, H., et all. . A&A . 526-105 . 2011 . 2011A&A...526A.105Z ,
Radial profiles of Fe abundance in the intracluster medium of nearby clusters observed with XMM-Newton . Matsushita, K., . A&A . 527-134 . 2011 . 2011A&A...527A.134M ,
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 ,
An Extremely Luminous Panchromatic Outburst from the Nucleus of a Distant Galaxy . Levan, A. J., Tanvir, N. R., et all. . Sci . 333-199 . 2011 . 2011Sci...333..199L ,
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 ,
The Swift Burst Alert Telescope Perspective on Non-thermal Emission in HIFLUGCS Galaxy Clusters . Wik, Daniel R., Sarazin, Craig L., et all. . ApJ . 748-67 . 2012 . 2012ApJ...748...67W ,
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 ,
Star-formation efficiency and metal enrichment of the intracluster medium in local massive clusters of galaxies . Zhang, Y.-Y., Laga...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2001-05-26T19:49:25Z/2001-05-27T05:02:53Z
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 2002-07-11T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2002-07-11T00:00:00Z, 006174, 17.56_20190403_1200. https://doi.org/10.5270/esa-h1vgpom