A dataset provided by the European Space Agency

Name 091681
Title Is the activity in the Milky Way disc sustaining the Galactic corona
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0916810101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0916810201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0916810301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0916810401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0916810501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0916810601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0916810701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0916810801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0916810901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0916811001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0916811201
...
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0916811401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0916811501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0916811701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0916811801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0916811901

DOI https://doi.org/10.57780/esa-7y6hjkr
Author European Space Agency
Description Covering the central 20*2.5deg2 of the Milky Way disc with 20ks XMM exposures
will allow us to measure the flows of hot baryons emerging from the energetic
activity in the disc, to detail their impact on the surroundings and to connect
the sources in the disc with the base of the Galactic outflow. By connecting the
requested XMM scan with the shallow all sky eROSITA survey, we will determine
whether the activity in the Galactic disc is important for feeding and
sustaining the Galactic corona. This study will provide us with an excellent
archetype for advancing our understanding of galaxy evolution theory in a
Milky-Way-class galaxy. This project will produce a legacy dataset that will be
used in the future for multiple purposes, including multi-wavelength and time-domain investigations.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2023-03-08T11:46:24Z/2023-09-29T17:54:20Z
Version 20.10_20230417_1156
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 2023-10-21T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2023, Is The Activity In The Milky Way Disc Sustaining The Galactic Corona, 20.10_20230417_1156, European Space Agency, https://doi.org/10.57780/esa-7y6hjkr