Matches in SemOpenAlex for { <https://semopenalex.org/work/W3040776951> ?p ?o ?g. }
Showing items 1 to 69 of
69
with 100 items per page.
- W3040776951 startingPage "1158" @default.
- W3040776951 abstract "The cloud RCW 95 was selected for study along with a number of other southern hemisphere regions in the galactic plane as part of a large program of search for YSOs associated with molecular clouds in the Galaxy. The project is an example of successful exploitation of large galactic surveys and combined both radio and far-IR observations. The selection of objects for study was based on data from the IRAS point source catalogue, in which we looked for sources with properties characteristic of star formation regions (SFRs). The main criteria constituted the presence of IRAS colours characteristic of compact HII regions, as according to work by Wood and Churchwell (1989) and the association with strong CS emission (using data from the catalogue of Bronfman et al. 1996). The presence of different maser species, typically found in association with SFRs, and ammonia lines was also used as an auxiliary information in the process. After selection, the stellar population of the regions were studied in the near-IR using data from both the 2MASS project and the SPTIZER satellite, allowing the construction of complete near-IR SEDs of the stars. RCW 95 is a special example of a region where the search successfully resulted in the discovery of several rich sites of star formation (Roman-Lopes and Abraham 2004 and 2006) and so, more detailed observations of the cloud were performed in radio in order to adress the structure and distribution of the compact HII regions therein. The continuum emission of the cloud was mapped in 43 GHz with a resolution of 2’ and a complete water maser survey was conducted in its direction, at 22.2 GHz, with a positional accuracy of 1’; the result of these observations was a more clear picture of the structure of the compact and ultracompact HII regions within the cloud and the discovery of more sites of star-formation that are still too obscured to be directly detected in the far-IR. In particular, the IRAS source 15412-5359 was revealed to be a compact site of massive star formation surrounded by an ionized region (powered by an O9V and several B0V stars) with a 43 GHz flux upper limit of 2.5 Jy." @default.
- W3040776951 created "2020-07-16" @default.
- W3040776951 creator A5017818858 @default.
- W3040776951 creator A5019203618 @default.
- W3040776951 creator A5022686161 @default.
- W3040776951 date "2006-01-01" @default.
- W3040776951 modified "2023-09-23" @default.
- W3040776951 title "Radio observations of the HII region complex RCW 95" @default.
- W3040776951 hasPublicationYear "2006" @default.
- W3040776951 type Work @default.
- W3040776951 sameAs 3040776951 @default.
- W3040776951 citedByCount "0" @default.
- W3040776951 crossrefType "journal-article" @default.
- W3040776951 hasAuthorship W3040776951A5017818858 @default.
- W3040776951 hasAuthorship W3040776951A5019203618 @default.
- W3040776951 hasAuthorship W3040776951A5022686161 @default.
- W3040776951 hasConcept C121332964 @default.
- W3040776951 hasConcept C125857072 @default.
- W3040776951 hasConcept C1276947 @default.
- W3040776951 hasConcept C144024400 @default.
- W3040776951 hasConcept C149923435 @default.
- W3040776951 hasConcept C150846664 @default.
- W3040776951 hasConcept C183582522 @default.
- W3040776951 hasConcept C2908647359 @default.
- W3040776951 hasConcept C44870925 @default.
- W3040776951 hasConcept C46061668 @default.
- W3040776951 hasConcept C86021447 @default.
- W3040776951 hasConcept C98444146 @default.
- W3040776951 hasConceptScore W3040776951C121332964 @default.
- W3040776951 hasConceptScore W3040776951C125857072 @default.
- W3040776951 hasConceptScore W3040776951C1276947 @default.
- W3040776951 hasConceptScore W3040776951C144024400 @default.
- W3040776951 hasConceptScore W3040776951C149923435 @default.
- W3040776951 hasConceptScore W3040776951C150846664 @default.
- W3040776951 hasConceptScore W3040776951C183582522 @default.
- W3040776951 hasConceptScore W3040776951C2908647359 @default.
- W3040776951 hasConceptScore W3040776951C44870925 @default.
- W3040776951 hasConceptScore W3040776951C46061668 @default.
- W3040776951 hasConceptScore W3040776951C86021447 @default.
- W3040776951 hasConceptScore W3040776951C98444146 @default.
- W3040776951 hasLocation W30407769511 @default.
- W3040776951 hasOpenAccess W3040776951 @default.
- W3040776951 hasPrimaryLocation W30407769511 @default.
- W3040776951 hasRelatedWork W1550196483 @default.
- W3040776951 hasRelatedWork W1555857659 @default.
- W3040776951 hasRelatedWork W1619000567 @default.
- W3040776951 hasRelatedWork W1975164695 @default.
- W3040776951 hasRelatedWork W2058750192 @default.
- W3040776951 hasRelatedWork W2099813013 @default.
- W3040776951 hasRelatedWork W2107221178 @default.
- W3040776951 hasRelatedWork W2123530368 @default.
- W3040776951 hasRelatedWork W2157510349 @default.
- W3040776951 hasRelatedWork W2158159714 @default.
- W3040776951 hasRelatedWork W2163978332 @default.
- W3040776951 hasRelatedWork W2166864331 @default.
- W3040776951 hasRelatedWork W2512415980 @default.
- W3040776951 hasRelatedWork W2942163845 @default.
- W3040776951 hasRelatedWork W2949205828 @default.
- W3040776951 hasRelatedWork W3036699304 @default.
- W3040776951 hasRelatedWork W3103554658 @default.
- W3040776951 hasRelatedWork W3104549047 @default.
- W3040776951 hasRelatedWork W3104621534 @default.
- W3040776951 hasRelatedWork W54852817 @default.
- W3040776951 hasVolume "77" @default.
- W3040776951 isParatext "false" @default.
- W3040776951 isRetracted "false" @default.
- W3040776951 magId "3040776951" @default.
- W3040776951 workType "article" @default.