A dataset provided by the European Space Agency

Name: A legacy survey of WR binaries - Part III
Published: 2021-04-16T00:00:00Z

Proposal ID	084021
Title	A legacy survey of WR binaries - Part III
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0840210101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0840210201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0840210301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0840210401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0840210501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0840210601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0840210701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0840210801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0840211101
DOI	https://doi.org/10.5270/esa-sz5tari
Principal Investigator, PI	Dr Yael Naze
Abstract	We propose to continue our magnitude-limited survey of well-known WR binariesthat were never observed in X-rays. This detection experiment aims at improvingthe knowledge of the X-ray emission of colliding wind systems in a variety ofsituations (i.e. spanning a range of different stellar and orbital parameters).It has a legacy value, as such detections are the starting point of detailedstudies.
Publications	New X-ray detections of known Wolf-Rayet stars \|Nazu00e9 Yau00ebl Gosset Eric \| MNRAS \| 501-4214 \| 2021 \| 2021MNRAS.501.4214N \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.501.4214N Colliding winds in WR21 and WR31 - I. The X-ray view \|Nazu00e9 Yau00ebl Rauw Gregor et al. \| MNRAS \| 526-2167 \| 2023 \| 2023MNRAS.526.2167N \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.526.2167N The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII O VIII and Fe L-shell Transitions \|Pan Zeyang Qu Zhijie et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez Antonio C. \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2019-10-03T15:56:11Z/2020-04-02T13:53:09Z
Version	18.02_20200221_1200
Mission Description	The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs 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 Earths 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	2021-04-16T00:00:00Z
Last Update	2025-01-27
Keywords	"colliding wind systems", "orbital parameters", "detection experiment aims", "magnitude limited survey", "xray emission", "wr binary"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Yael Naze, 2021, 'A legacy survey of WR binaries - Part III', 18.02_20200221_1200, European Space Agency, https://doi.org/10.5270/esa-sz5tari