Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/32801| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Xu, Y. | en_US |
| dc.contributor.author | Reid, M. J. | en_US |
| dc.contributor.author | Menten, K. M. | en_US |
| dc.contributor.author | Brunthaler, A. | en_US |
| dc.contributor.author | Zheng, X. W. | en_US |
| dc.contributor.author | MOSCADELLI, Luca | en_US |
| dc.date.accessioned | 2022-12-27T13:55:33Z | - |
| dc.date.available | 2022-12-27T13:55:33Z | - |
| dc.date.issued | 2007 | en_US |
| dc.identifier.isbn | 978-0521-87464-9 | en_US |
| dc.identifier.issn | 1743-9213 | en_US |
| dc.identifier.uri | http://hdl.handle.net/20.500.12386/32801 | - |
| dc.description.abstract | We have measured the distance to the high-mass star-forming region G59.7+0.1, which harbors the far-infra-red source IRAS 19410+2336. The distance is 2.20 ± 0.11 kpc and was determined by triangulation using Very Long Baseline Array (VLBA) observations of 12.2 GHz methanol masers phase-referenced to two compact extragalactic radio sources. | en_US |
| dc.language.iso | eng | en_US |
| dc.title | The distance to G59.7+0.1 | en_US |
| dc.type | Conference paper | - |
| dc.identifier.doi | 10.1017/S1743921307013403 | en_US |
| dc.identifier.scopus | 2-s2.0-38849083927 | en_US |
| dc.identifier.url | https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/distance-to-g59701/DD3EC1623C9774454DFB62C301A9778A | en_US |
| dc.identifier.url | https://api.elsevier.com/content/abstract/scopus_id/38849083927 | en_US |
| dc.relation.medium | ELETTRONICO | en_US |
| dc.relation.volume | 242 | en_US |
| dc.relation.firstpage | 374 | en_US |
| dc.relation.lastpage | 375 | en_US |
| dc.type.referee | REF_3 | en_US |
| dc.description.numberofauthors | 6 | 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 | Chapman, Jessica M.; Baan, Willem A. | en_US |
| dc.relation.ispartofbook | Astrophysical Masers and their Environments | 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 | Astrophysical Masers and their Environments | en_US |
| dc.relation.conferenceplace | Alice Springs, Australia | en_US |
| dc.relation.conferencedate | March 12-16, 2007 | 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 | 2007IAUS..242..374X | 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.grantfulltext | open | - |
| item.languageiso639-1 | en | - |
| item.fulltext | With Fulltext | - |
| item.openairetype | Conference paper | - |
| item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
| item.cerifentitytype | Publications | - |
| crisitem.journal.journalissn | 1743-9213 | - |
| crisitem.journal.ance | E192651 | - |
| crisitem.author.dept | O.A. Arcetri | - |
| crisitem.author.orcid | 0000-0002-8517-8881 | - |
| Appears in Collections: | 3.01 Contributi in Atti di convegno | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| Xu_2007_IAUS.pdf | PDF editoriale | 196.52 kB | Adobe PDF | View/Open |
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