A dataset provided by the European Space Agency

Name 040266
Title XMM monitoring of the Seyfert Galaxy NGC 4151: Probing the Disk-Wind Connection
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0402660101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0402660201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0402660301

DOI 10.5270/esa-h79ziov
Author Prof Steven Kraemer
Description Recent X-ray observations of NGC 4151 have revealed dramatic changes in the X-ray absorption due to bulk motion of the gas across our line-of-sight. Based on photoionization models, much of this component must lie within 0.1 pc of the central source, which, combined with the large transverse velocity, suggests that the absorber arises in a disk-driven wind, making NGC 4151 the only Seyfert 1 to have shown direct evidence of this phenomenon. We propose a series of 4 new XMM-Newton observations of NGC 4151, of 40 ksec each, to fully constrain the kinematics, location, and physical conditions of the high-column X-ray aborber, and probe the relative effects of radiation driving, thermal pressure, and magnetocentrifugal forces in accelerating the gas.
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Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2006-05-16T06:21:42Z/2006-11-30T11:02:58Z
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 2008-01-25T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2008-01-25T00:00:00Z, 040266, 17.56_20190403_1200. https://doi.org/10.5270/esa-h79ziov