Skip navigation
  • INAF logo
  • Home
  • Communities
    & Collections
  • Research outputs
  • Researchers
  • Organization units
  • Projects
  • Explore by
    • Research outputs
    • Researchers
    • Organization units
    • Projects
  • Login:
    • My DSpace
    • Receive email
      updates
    • Edit Account details
  • Italian
  • English

  1. OA@INAF
  2. PRODOTTI RICERCA INAF
  3. 1 CONTRIBUTI IN RIVISTE (Journal articles)
  4. 1.01 Articoli in rivista
Please use this identifier to cite or link to this item: http://hdl.handle.net/20.500.12386/23908
DC FieldValueLanguage
dc.contributor.authorIODICE, ENRICHETTA-
dc.contributor.authorCapaccioli, M.-
dc.contributor.authorSPAVONE, MARILENA-
dc.contributor.authorNAPOLITANO, NICOLA ROSARIO-
dc.contributor.authorGRADO, ANIELLO-
dc.contributor.authorLimatola, L.-
dc.contributor.authorCANTIELLO, Michele-
dc.contributor.authorSCHIPANI, Pietro-
dc.date.accessioned2020-04-07T16:11:46Z-
dc.date.available2020-04-07T16:11:46Z-
dc.date.issued2015en_US
dc.identifier.issn0004-6361-
dc.identifier.urihttp://hdl.handle.net/20.500.12386/23908-
dc.descriptionWe are very grateful to the anonymous referee for his or her comments and suggestions that helped us to improve and clarify our work. This work was supported by the PRIN-INAF “Galaxy Evolution with the VLT Survey Telescope (VST)” (PI A. Grado). M. Cantiello acknowledges support from PO FSE Abruzzo 2007-2013 (PO 2012/2013).-
dc.description.abstractWe present the first deep photometry of what may be a good candidate for a forming polar-ring galaxy at redshift z ≃ 0.05. The object FCSS J033710.0-354727 is a background galaxy in the VST Deep Field of the Fornax cluster. The deep exposures combined with the high angular resolution of the OmegaCam at VST allowed us to carry out the first detailed photometric analysis for this system in the g and i bands to derive the galaxy structure and colors. Results show that the central object resembles a disk galaxy, surrounded by a ring-like structure that is twice as extended as the central disk. The warped geometry and bright knots observed along the polar direction, as well as some debris detected on the NW side with colors similar to those of the galaxy, suggest that the polar structure is still forming. We argue that the wide polar ring or disk is the result of the ongoing disruption of a companion galaxy in the potential well of the central object, which is two to three times more massive than the accreting galaxy. <P />This work is based on observations taken at the ESO La Silla Paranal Observatory within the VST GTO Program ID 088.B-4012(A).-
dc.language.isoeng-
dc.titleA forming wide polar-ring galaxy at z ~ 0.05 in the VST Deep Field of the Fornax clusteren_US
dc.typeArticle-
dc.identifier.doi10.1051/0004-6361/201425263en_US
dc.identifier.scopus2-s2.0-84922224854en_US
dc.identifier.isi000349467000111en_US
dc.identifier.urlhttps://www.aanda.org/articles/aa/abs/2015/02/aa25263-14/aa25263-14.html-
dc.relation.mediumSTAMPA-
dc.relation.volume574-
dc.relation.firstpageA111-
dc.type.refereeREF_1-
dc.description.internationalsì-
dc.relation.scientificsectorFIS/05 - ASTRONOMIA E ASTROFISICA-
dc.relation.journalASTRONOMY & ASTROPHYSICS-
dc.type.miur262 Articolo in rivista-
dc.identifier.adsbibcode2015A&A...574A.111I-
dc.description.apcno-
dc.description.oa1 – prodotto con file in versione Open Access (allegherò il file al passo  5-Carica)-
item.grantfulltextopen-
item.languageiso639-1en-
item.fulltextWith Fulltext-
item.openairetypeArticle-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.cerifentitytypePublications-
crisitem.journal.journalissn0004-6361-
crisitem.journal.anceE016240-
crisitem.author.deptO.A. Capodimonte-
crisitem.author.deptO.A. Capodimonte-
crisitem.author.deptO.A. Capodimonte-
crisitem.author.deptO.A. Capodimonte-
crisitem.author.deptO.A. Abruzzo-
crisitem.author.deptO.A. Capodimonte-
crisitem.author.orcid0000-0003-4291-0005-
crisitem.author.orcid0000-0002-6427-7039-
crisitem.author.orcid0000-0003-0911-8884-
crisitem.author.orcid0000-0002-0501-8256-
crisitem.author.orcid0000-0003-2072-384X-
crisitem.author.orcid0000-0003-0197-589X-
Appears in Collections:1.01 Articoli in rivista
Files in This Item:
File Description SizeFormat
aa25263-14.pdfPdf editoriale11.81 MBAdobe PDFView/Open
23908-aa25263-14_P01.pdfMiur8.54 MBAdobe PDF
23908-aa25263-14_P02.pdfMiur3.26 MBAdobe PDF
Show simple item record

Page view(s)

74
checked on Jun 9, 2023

Download(s)

14
checked on Jun 9, 2023

Google ScholarTM

Check

Altmetric

Altmetric


Items in DSpace are published in Open Access, unless otherwise indicated.


Explore by
  • Communities
    & Collections
  • Research outputs
  • Researchers
  • Organization units
  • Projects

Informazioni e guide per autori

https://openaccess-info.inaf.it: tutte le informazioni sull'accesso aperto in INAF

Come si inserisce un prodotto: le guide a OA@INAF

La Policy INAF sull'accesso aperto

Documenti e modelli scaricabili

Feedback
Built with DSpace-CRIS - Extension maintained and optimized by Logo 4SCIENCE