Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/23879
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Konyves, V. | en_US |
dc.contributor.author | Andre, P. | en_US |
dc.contributor.author | Men'shchikov, A. | en_US |
dc.contributor.author | Palmeirim, P. | en_US |
dc.contributor.author | Arzoumanian, D. | en_US |
dc.contributor.author | Schneider, N. | en_US |
dc.contributor.author | RYGL, Kazi Lucie Jessica | en_US |
dc.contributor.author | Didelon, P. | en_US |
dc.contributor.author | Maury, A. | en_US |
dc.contributor.author | Shimajiri, Y. | en_US |
dc.contributor.author | Di, Francesco J. | en_US |
dc.contributor.author | Bontemps, S. | en_US |
dc.contributor.author | Peretto, N. | en_US |
dc.contributor.author | BENEDETTINI, Milena | en_US |
dc.contributor.author | Bernard, J. -P. | en_US |
dc.contributor.author | ELIA, Davide Quintino | en_US |
dc.contributor.author | Griffin, M. J. | en_US |
dc.contributor.author | Hill, T. | en_US |
dc.contributor.author | Kirk, J. | en_US |
dc.contributor.author | Ladjelate, B. | en_US |
dc.contributor.author | Marsh, K. | en_US |
dc.contributor.author | Martin, P. G. | en_US |
dc.contributor.author | Motte, F. | en_US |
dc.contributor.author | Nguyen Luong, Q. | en_US |
dc.contributor.author | PEZZUTO, Stefano | en_US |
dc.contributor.author | Roussel, H. | en_US |
dc.contributor.author | Sadavoy, S. I. | en_US |
dc.contributor.author | SCHISANO, EUGENIO | en_US |
dc.contributor.author | SPINOGLIO, Luigi Giuseppe Maria | en_US |
dc.contributor.author | Ward-Thompson, D. | en_US |
dc.contributor.author | White, G. J. | en_US |
dc.date.accessioned | 2020-04-06T14:43:51Z | - |
dc.date.available | 2020-04-06T14:43:51Z | - |
dc.date.issued | 2015 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/23879 | - |
dc.description.abstract | Based on Herschel Gould Belt survey (Andre et al., 2010A&A...518L.102A) observations of the Aquila cloud complex, and using the multi-scale, multi-wavelength source extraction algorithm getsources (Men'shchikov et al., 2012A&A...542A..81M), we identified a total of 749 dense cores, including 685 starless cores and 64 protostellar cores. The observed properties of all dense cores are given in tablea1.dat, and their derived properties are listed in tablea2.dat. (4 data files). | en_US |
dc.language.iso | eng | en_US |
dc.title | VizieR Online Data Catalog: Catalog of dense cores in Aquila from Herschel (Konyves+, 2015) | en_US |
dc.type | Database | - |
dc.identifier.doi | 10.26093/cds/vizier.35840091 | en_US |
dc.identifier.url | http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/A+A/584/A91 | en_US |
dc.relation.firstpage | J/A+A/584/A91 | - |
dc.description.numberofauthors | 32 | en_US |
dc.description.international | sì | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | VizieR Online Data Catalog | - |
dc.type.miur | 295 Banca dati | - |
dc.identifier.adsbibcode | 2015yCat..35840091K | - |
dc.description.oa | 3 – prodotto già presente in altro archivio Open Access (arXiv, REPEC…) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.grantfulltext | open | - |
item.languageiso639-1 | en | - |
item.openairetype | Database | - |
item.cerifentitytype | Publications | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.orcid | 0000-0003-4146-9043 | - |
crisitem.author.orcid | 0000-0002-3597-7263 | - |
crisitem.author.orcid | 0000-0002-9120-5890 | - |
crisitem.author.orcid | 0000-0001-7852-1971 | - |
crisitem.author.orcid | 0000-0003-1560-3958 | - |
crisitem.author.orcid | 0000-0001-8840-1551 | - |
Appears in Collections: | 4.06 Banche Dati |
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File | Description | Size | Format | |
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J_A+A_584_A91.pdf | ReadMe | 168.21 kB | Adobe PDF | View/Open |
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