Matches in SemOpenAlex for { <https://semopenalex.org/work/W2149026051> ?p ?o ?g. }
- W2149026051 abstract "A survey of young bipolar outflows in regions of low-to-intermediate-mass star formation has been carried out in two Class I methanol maser transitions: 70− 61A+ at 44 GHz and 4−1− 30E at 36 GHz. We detected narrow features towards NGC 1333I2A, NGC 1333I4A, HH25MMS and L1157 at 44 GHz, and towards NGC 2023 at 36 GHz. Flux densities of the lines detected at 44 GHz are no higher than 11 Jy and the relevant source luminosities are about 1022 erg s−1, which is much lower than those of strong masers in high-mass star formation regions. No emission was found towards 39 outflows. All masers detected at 44 GHz are located in clouds with methanol column densities of the order of or larger than a few ×1014 cm−2. The upper limits for the non-detections are typically of the order of 3–5 Jy. Observations in 2004, 2006 and 2008 did not reveal any significant variability of the 44 GHz masers in NGC 1333I4A, HH25MMS and L1157." @default.
- W2149026051 created "2016-06-24" @default.
- W2149026051 creator A5026224896 @default.
- W2149026051 creator A5040797424 @default.
- W2149026051 creator A5054798676 @default.
- W2149026051 creator A5058683818 @default.
- W2149026051 creator A5064768265 @default.
- W2149026051 creator A5070356403 @default.
- W2149026051 creator A5076502558 @default.
- W2149026051 date "2010-04-01" @default.
- W2149026051 modified "2023-10-16" @default.
- W2149026051 title "Search for Class I methanol masers in low-mass star formation regions" @default.
- W2149026051 cites W1965520676 @default.
- W2149026051 cites W1971036004 @default.
- W2149026051 cites W1971943380 @default.
- W2149026051 cites W1975702842 @default.
- W2149026051 cites W1977920199 @default.
- W2149026051 cites W1993330702 @default.
- W2149026051 cites W1997566741 @default.
- W2149026051 cites W2004167413 @default.
- W2149026051 cites W2008534099 @default.
- W2149026051 cites W2010268922 @default.
- W2149026051 cites W2018397605 @default.
- W2149026051 cites W2023002681 @default.
- W2149026051 cites W2023055517 @default.
- W2149026051 cites W2024023618 @default.
- W2149026051 cites W2030406463 @default.
- W2149026051 cites W2033647522 @default.
- W2149026051 cites W2036326185 @default.
- W2149026051 cites W2040522531 @default.
- W2149026051 cites W2041964794 @default.
- W2149026051 cites W2042178638 @default.
- W2149026051 cites W2043647577 @default.
- W2149026051 cites W2049862045 @default.
- W2149026051 cites W2051660968 @default.
- W2149026051 cites W2062760730 @default.
- W2149026051 cites W2063189458 @default.
- W2149026051 cites W2070005605 @default.
- W2149026051 cites W2071142800 @default.
- W2149026051 cites W2074513601 @default.
- W2149026051 cites W2078092087 @default.
- W2149026051 cites W2081775518 @default.
- W2149026051 cites W2084219470 @default.
- W2149026051 cites W2085294935 @default.
- W2149026051 cites W2086077065 @default.
- W2149026051 cites W2098234176 @default.
- W2149026051 cites W2105756122 @default.
- W2149026051 cites W2110711701 @default.
- W2149026051 cites W2132203097 @default.
- W2149026051 cites W2138991917 @default.
- W2149026051 cites W2149465673 @default.
- W2149026051 cites W2160788465 @default.
- W2149026051 cites W2163640162 @default.
- W2149026051 cites W2164154779 @default.
- W2149026051 cites W2166670154 @default.
- W2149026051 cites W2169248318 @default.
- W2149026051 cites W3101988869 @default.
- W2149026051 cites W3104901630 @default.
- W2149026051 cites W3106445853 @default.
- W2149026051 cites W3106482143 @default.
- W2149026051 doi "https://doi.org/10.1111/j.1365-2966.2010.16484.x" @default.
- W2149026051 hasPublicationYear "2010" @default.
- W2149026051 type Work @default.
- W2149026051 sameAs 2149026051 @default.
- W2149026051 citedByCount "22" @default.
- W2149026051 countsByYear W21490260512012 @default.
- W2149026051 countsByYear W21490260512013 @default.
- W2149026051 countsByYear W21490260512014 @default.
- W2149026051 countsByYear W21490260512015 @default.
- W2149026051 countsByYear W21490260512017 @default.
- W2149026051 countsByYear W21490260512018 @default.
- W2149026051 countsByYear W21490260512019 @default.
- W2149026051 crossrefType "journal-article" @default.
- W2149026051 hasAuthorship W2149026051A5026224896 @default.
- W2149026051 hasAuthorship W2149026051A5040797424 @default.
- W2149026051 hasAuthorship W2149026051A5054798676 @default.
- W2149026051 hasAuthorship W2149026051A5058683818 @default.
- W2149026051 hasAuthorship W2149026051A5064768265 @default.
- W2149026051 hasAuthorship W2149026051A5070356403 @default.
- W2149026051 hasAuthorship W2149026051A5076502558 @default.
- W2149026051 hasBestOaLocation W21490260511 @default.
- W2149026051 hasConcept C121332964 @default.
- W2149026051 hasConcept C125857072 @default.
- W2149026051 hasConcept C1276947 @default.
- W2149026051 hasConcept C150846664 @default.
- W2149026051 hasConcept C191897082 @default.
- W2149026051 hasConcept C192562407 @default.
- W2149026051 hasConcept C2780897414 @default.
- W2149026051 hasConcept C3017610826 @default.
- W2149026051 hasConcept C44870925 @default.
- W2149026051 hasConcept C46061668 @default.
- W2149026051 hasConcept C68709404 @default.
- W2149026051 hasConceptScore W2149026051C121332964 @default.
- W2149026051 hasConceptScore W2149026051C125857072 @default.
- W2149026051 hasConceptScore W2149026051C1276947 @default.
- W2149026051 hasConceptScore W2149026051C150846664 @default.
- W2149026051 hasConceptScore W2149026051C191897082 @default.
- W2149026051 hasConceptScore W2149026051C192562407 @default.
- W2149026051 hasConceptScore W2149026051C2780897414 @default.
- W2149026051 hasConceptScore W2149026051C3017610826 @default.