A dataset provided by the European Space Agency

Name 030617
Title A NEW CLASS OF HIGHLY ABSORBED PERSISTENT HMXB
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0306170201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0306170401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0306170901
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0306171201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0306172001

DOI 10.5270/esa-hxfknyc
Author Dr Roland Walter
Description To date more than 40 new bright hard X-ray Galactic plane sources have been discovered with INTEGRAL, and 10 of them have follow-up observations with XMM-Newton or Chandra. In most cases, the X-ray data exhibit slow pulsations, and the absorbing column density appear much larger than expected in the Galaxy or in front of the companion star. Many of those sources are persistent and seem to belong to a new class of HMXB, with a slow pulsar orbiting in a dense circumstellar material or within the companion stellar envelope itself. The goal of this proposal is twofold. We propose (1) to observe several additional persistent new INTEGRAL sources and (2) to study more in depth a few already studied sources.
Publication The broad-band XMM-Newton and INTEGRAL spectra of bright type 1 Seyfert galaxies . Panessa, F., Bassani, L., et all. . A&A . 483-151 . 2008 . 2008A&A...483..151P ,
INTEGRAL and XMM-Newton observations of AX J1845.0-0433 . Zurita Heras, J. A., Walter, R., . A&A . 494-1013 . 2009 . 2009A&A...494.1013Z ,
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 ,
The INTEGRAL complete sample of type 1 AGN . Molina, M., Bassani, L., et all. . MNRAS . 399-1293 . 2009 . 2009MNRAS.399.1293M ,
IGR J17254-3257, a new bursting neutron star . Chenevez, J., Falanga, M., et all. . A&A . 469-27 . 2007 . 2007A&A...469L..27C ,
Discovery of an Energetic 38.5 ms Pulsar Powering the Gamma-ray Source IGR J18490-0000-HESS J1849-000 . Gotthelf, E. V., Halpern, J. P., et all. . ApJ . 729-16 . 2011 . 2011ApJ...729L..16G ,
The Galactic plane at faint X-ray fluxes - I. Properties and characteristics of the X-ray source population . Warwick, R. S., Perez-Ramirez, D., . MNRAS . 413-595 . 2011 . 2011MNRAS.413..595W ,
Fe Kalpha line profile in AGNs: average shape and redshift dependence . Mao, Wei-Ming, Hu, Chen, et all. . RAA . 10-905 . 2010 . 2010RAA....10..905M ,
Searching for X-ray emission from ...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2006-03-01T04:26:07Z/2006-04-04T00:34:14Z
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 2007-05-31T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2007-05-31T00:00:00Z, 030617, 17.56_20190403_1200. https://doi.org/10.5270/esa-hxfknyc