Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/32792
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Li, J. J. | en_US |
dc.contributor.author | MOSCADELLI, Luca | en_US |
dc.contributor.author | CESARONI, Riccardo | en_US |
dc.contributor.author | Furuya, R. S. | en_US |
dc.contributor.author | Xu, Y. | en_US |
dc.contributor.author | Usuda, T. | en_US |
dc.contributor.author | Menten, K. M. | en_US |
dc.contributor.author | Pestalozzi, M. | en_US |
dc.contributor.author | ELIA, Davide Quintino | en_US |
dc.contributor.author | SCHISANO, EUGENIO | en_US |
dc.date.accessioned | 2022-12-20T16:14:19Z | - |
dc.date.available | 2022-12-20T16:14:19Z | - |
dc.date.issued | 2012 | en_US |
dc.identifier.isbn | 9781107032842 | en_US |
dc.identifier.issn | 1743-9213 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/32792 | - |
dc.description.abstract | We investigated the high-mass star-forming region G28.87+0.07 by means of maser kinematics, including H<SUB>2</SUB>O, CH<SUB>3</SUB>OH, and OH, and radio to infrared, continuum observations. All observational evidence suggests that these masers are associated with the same young star of 20-30 M<SUB>⊙</SUB>, still in the main accretion phase and surrounded by a rich stellar cluster. | en_US |
dc.language.iso | eng | en_US |
dc.title | Massive star-formation toward G28.87+0.07 | en_US |
dc.type | Conference paper | - |
dc.identifier.doi | 10.1017/S1743921312006898 | en_US |
dc.identifier.scopus | 2-s2.0-84864429912 | en_US |
dc.identifier.url | https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/massive-starformation-toward-g2887007/7655978F455BC30124895E5EE7C4282B | en_US |
dc.identifier.url | https://api.elsevier.com/content/abstract/scopus_id/84864429912 | en_US |
dc.relation.medium | ELETTRONICO | en_US |
dc.relation.volume | vol. 8, S287 | en_US |
dc.relation.firstpage | 180 | en_US |
dc.relation.lastpage | 181 | en_US |
dc.type.referee | REF_3 | en_US |
dc.description.numberofauthors | 10 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | USA | en_US |
dc.contributor.country | DEU | en_US |
dc.contributor.country | CHN | en_US |
dc.relation.alleditors | Booth, R.S.; Humphreys, E.M.L.; Vilemmings, W.H.T. | en_US |
dc.relation.ispartofbook | Cosmic Masers - from OH to H0 | en_US |
dc.publisher.name | Cambridge University Press. | en_US |
dc.publisher.country | GBR | en_US |
dc.relation.conferencename | Cosmic Masers - from OH to H0 | en_US |
dc.relation.conferenceplace | Stellenbosch, South Africa | en_US |
dc.relation.conferencedate | 29 January- 3 February, 2012 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.type.miur | 273 Contributo in Atti di convegno | - |
dc.relation.series | PROCEEDINGS OF THE INTERNATIONAL ASTRONOMICAL UNION | en_US |
dc.identifier.adsbibcode | 2012IAUS..287..180L | 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 | Conference paper | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.orcid | 0000-0002-8517-8881 | - |
crisitem.author.orcid | 0000-0002-2430-5103 | - |
crisitem.author.orcid | 0000-0002-9120-5890 | - |
crisitem.author.orcid | 0000-0003-1560-3958 | - |
crisitem.journal.journalissn | 1743-9213 | - |
crisitem.journal.ance | E192651 | - |
Appears in Collections: | 3.01 Contributi in Atti di convegno |
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File | Description | Size | Format | |
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Li_2012_IAUS.pdf | PDF editoriale | 210.34 kB | Adobe PDF | View/Open |
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