A dataset provided by the European Space Agency

Name: Abell 1367: a nearby laboratory to study cluster merger and galaxy evolution
Published: 2019-06-14T22:00:00Z

Proposal ID	082320
Title	Abell 1367: a nearby laboratory to study cluster merger and galaxy evolution
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0823200101
DOI	https://doi.org/10.5270/esa-fh4musw
Principal Investigator, PI	Dr Ming Sun
Abstract	Both the ICM and galaxies have bulk motion inside clusters, providing clues onthe cluster dynamics. The interaction between the ICM and galaxies plays a vitalrole in galaxy evolution, dramatically shown by a stripping tail sometime. X-raytails of late-type cluster galaxies were only detected recently. Detailedstudies of these systems allow better understanding for ram- pressure stripping,galaxy transformation, mixing of the stripped cold ISM with the hot ICM,r^ant micro-physics and intracluster SF. In this proposal, we request XMMtime to study one of the X-ray brightest and the closest clusters A1367. It isan ideal system to study both X-ray tails (a new sample of Ha tails and richamount of multi-band data) and cluster merger (multiple merger events and at least one shock).
Publications	A merger shock in Abell 1367 \|Ge Chong Sun Ming et al. \| MNRAS \| 486-36 \| 2019 \| 2019MNRAS.486L..36G \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.486L..36G An H u03b1/X-ray orphan cloud as a signpost of intracluster medium clumping \|Ge Chong Luo Rongxin et al. \| MNRAS \| 505-4702 \| 2021 \| 2021MNRAS.505.4702G \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.505.4702G The BIG X-ray tail \|Ge Chong Sun Ming et al. \| MNRAS \| 508-69 \| 2021 \| 2021MNRAS.508L..69G \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.508L..69G Non-star-forming molecular gas in the Abell 1367 intra-cluster multiphase orphan cloud \|Ju00e1chym Pavel Sun Ming et al. \| A&A \| 658-5 \| 2022 \| 2022A&A...658L...5J \| http://ui.adsabs.harvard.edu/#abs/2022A&A...658L...5J A universal correlation between warm and hot gas in the stripped tails of cluster galaxies \|Sun Ming Ge Chong et al. \| NatAs \| 6-270 \| 2021 \| 2022NatAs...6..270S \| http://ui.adsabs.harvard.edu/#abs/2022NatAs...6..270S
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2018-06-01T03:47:41Z/2018-06-02T00:04:21Z
Version	17.56_20190403_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	2019-06-14T22:00:00Z
Last Update	2025-01-27
Keywords	"cluster merger", "relevant micro physics", "ideal system", "galaxy transformation", "ram pressure", "galaxy plays", "stripped cold ism", "ha tails", "multi band data", "xmm time", "galaxy evolution", "closest cluster a1367", "hot icm", "xray brightest", "intracluster sf", "vital role", "rich amount", "cluster dynamics", "nearby laboratory", "abell 1367 \:", "Abell 1367", "tail sometime", "xray tails", "XMM"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Ming Sun, 2019, 'Abell 1367: a nearby laboratory to study cluster merger and galaxy evolution', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-fh4musw