A dataset provided by the European Space Agency

Name 050335
Title An Exploratory Survey of NAL Quasars With High Velocity Outflows
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0503350101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0503350201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0503350301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0503350401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0503350501

DOI https://doi.org/10.5270/esa-f8u3wru
Author Dr George Chartas
Description Recent spectroscopic observations in the UV band have revealed high velocity
outflows in Narrow Absorption Line (NAL) quasars. We propose to initiate an
exploratory survey to identify high velocity outflows of X-ray absorbing
material in NAL quasars. We will search for possible correlations between the
amount of X-ray absorption and UV properties of the wind to better understand
the acceleration mechanism of quasar winds. We will place the absorbers of NAL
quasars in the context of other outflow phenomena and test models for their
nature. The detected X-ray brightest objects from the proposed survey will be
followed up with deeper observations to constrain better the kinematic and
ionization properties of the absorbers and ultimately constrain the mass outflow rates of NAL quasars.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2007-07-11T13:07:15Z/2007-10-31T12:16:59Z
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 2008-12-11T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr George Chartas, 2008, 050335, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-f8u3wru