A dataset provided by the European Space Agency

Name 011253
Title GT Observations of Hot Stars: Zeta Ori
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112530101

DOI https://doi.org/10.5270/esa-14fn2fw
Author Dr Albert Brinkman
Description GT-zeta Ori, a late O type supergiant, is a strong X-ray source. The X-rays
originate from shocks in the stellar wind. The observations will be used to
establish the physical conditions and elemental abundances in the shocked
material. With models of line transfer in moving atmospheres we will determine
the volume filling factor and depth distribution of the shocked gas pockets.
This will help to constrain the still unknown mechanism that triggers these
shocks. zeta Ori will be in the RGS focus. The surrounding field is a star
formation region with many X-ray sources. We will use the EPIC cameras to study
this complete field as well. The pn will be used in full window mode, one MOS
with window2 and the other MOS in timing mode. All EPICs will use the thick filter.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2002-09-15T13:12:07Z/2002-09-16T00:52:19Z
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 2003-10-10T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Albert Brinkman, 2003, 011253, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-14fn2fw