Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/26538
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Sereno, Mauro | en_US |
dc.contributor.author | ETTORI, STEFANO | en_US |
dc.contributor.author | MENEGHETTI, MASSIMO | en_US |
dc.contributor.author | Sayers, Jack | en_US |
dc.contributor.author | Umetsu, Keiichi | en_US |
dc.contributor.author | MERTEN, JULIAN | en_US |
dc.contributor.author | Chiu, I. -Non | en_US |
dc.contributor.author | Zitrin, Adi | en_US |
dc.date.accessioned | 2020-07-21T06:32:59Z | - |
dc.date.available | 2020-07-21T06:32:59Z | - |
dc.date.issued | 2017 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/26538 | - |
dc.description.abstract | Multi-wavelength techniques can probe the distribution and the physical properties of baryons and dark matter in galaxy clusters from the inner regions out to the peripheries. We present a full three-dimensional analysis combining strong and weak lensing, X-ray surface brightness and temperature, and the Sunyaev-Zel'dovich effect. The method is applied to MACS J1206.2-0847, a remarkably regular, face-on, massive, M<SUB>200</SUB> = (1.1 ± 0.2) × 10<SUP>15</SUP> M<SUB>☉</SUB> h<SUP>-1</SUP>, cluster at z = 0.44. The measured concentration, c<SUB>200</SUB> = 6.3 ± 1.2, and the triaxial shape are common to haloes formed in a Λ cold dark matter scenario. The gas has settled in and follows the shape of the gravitational potential, which is evidence of pressure equilibrium via the shape theorem. There is no evidence for significant non-thermal pressure and the equilibrium is hydrostatic. | en_US |
dc.language.iso | eng | en_US |
dc.title | CLUMP-3D: three-dimensional lensing and multi-probe analysis of MACS J1206.2-0847, a remarkably regular cluster | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/stx326 | en_US |
dc.identifier.scopus | 2-s2.0-85020689902 | en_US |
dc.identifier.isi | 000398421100003 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/article/467/4/3801/2973011 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 467 | en_US |
dc.relation.issue | 4 | en_US |
dc.relation.firstpage | 3801 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 8 | en_US |
dc.description.international | sì | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | en_US |
dc.type.miur | 262 Articolo in rivista | en_US |
dc.identifier.adsbibcode | 2017MNRAS.467.3801S | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation::PE9_6 Stars and stellar systems | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Article | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.orcid | 0000-0003-0302-0325 | - |
crisitem.author.orcid | 0000-0003-4117-8617 | - |
crisitem.author.orcid | 0000-0003-1225-7084 | - |
crisitem.journal.journalissn | 0035-8711 | - |
crisitem.journal.ance | E112946 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
CLUMP-3D-MACS J1206.2-0847.pdf | PDF editoriale | 6.22 MB | Adobe PDF | View/Open |
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