Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/32791
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Xu, Y. | en_US |
dc.contributor.author | Reid, M. J. | en_US |
dc.contributor.author | MOSCADELLI, Luca | en_US |
dc.contributor.author | Menten, K. M. | en_US |
dc.contributor.author | Zheng, X. W. | en_US |
dc.contributor.author | Brunthaler, A. | en_US |
dc.contributor.author | Zhang, B. | en_US |
dc.contributor.author | RYGL, Kazi Lucie Jessica | en_US |
dc.contributor.author | Li, J. J. | en_US |
dc.contributor.author | SANNA, ALBERTO | en_US |
dc.date.accessioned | 2022-12-20T15:45:23Z | - |
dc.date.available | 2022-12-20T15:45:23Z | - |
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/20.500.12386/32791 | - |
dc.description.abstract | Due to their compactness, persistence and slow motion, Class II CH<SUB>3</SUB>OH masers are excellent targets for parallax and proper motion measurements for massive star-forming regions in the Galactic Disk. These measurements can be used to improve our understanding of the spiral structure and dynamics of the Milky Way. At the same time, Class II CH<SUB>3</SUB>OH masers can also be used to study gas kinematics close to the exciting star, tracing rotation, infall and/or outflow motions. | en_US |
dc.language.iso | eng | en_US |
dc.title | Methanol Maser Parallaxes and Proper Motions | en_US |
dc.type | Conference paper | - |
dc.identifier.doi | 10.1017/S1743921312007326 | en_US |
dc.identifier.scopus | 2-s2.0-84864475743 | en_US |
dc.identifier.url | https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/methanol-maser-parallaxes-and-proper-motions/D9E30BC4ABCD73352ED745FCB4A12A20 | en_US |
dc.identifier.url | https://api.elsevier.com/content/abstract/scopus_id/84864475743 | en_US |
dc.relation.medium | ELETTRONICO | en_US |
dc.relation.volume | vol. 8, S287 | en_US |
dc.relation.firstpage | 368 | en_US |
dc.relation.lastpage | 376 | 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 | NLD | 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.type.invited | no | 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..368X | en_US |
dc.description.apc | sì | 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 | IRA Bologna | - |
crisitem.author.dept | O.A. Cagliari | - |
crisitem.author.orcid | 0000-0002-8517-8881 | - |
crisitem.author.orcid | 0000-0003-4146-9043 | - |
crisitem.author.orcid | 0000-0001-7960-4912 | - |
crisitem.journal.journalissn | 1743-9213 | - |
crisitem.journal.ance | E192651 | - |
Appears in Collections: | 3.01 Contributi in Atti di convegno |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
Xu_2012_IAUS.pdf | PDF editoriale | 1.12 MB | Adobe PDF | View/Open |
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