Publication:
Mopra observations of G305.2+0.2: massive star formation at different evolutionary stages?
Mopra observations of G305.2+0.2: massive star formation at different evolutionary stages?
dc.contributor.author | Walsh, Andrew | en_US |
dc.contributor.author | Burton, Michael | en_US |
dc.date.accessioned | 2021-11-25T12:54:45Z | |
dc.date.available | 2021-11-25T12:54:45Z | |
dc.date.issued | 2006 | en_US |
dc.description.abstract | We have successfully used a new on-the-fly mapping technique with the Mopra radio telescope to image G305.2+0.2 in transitions of (CO)-C-13, HCO+, N2H+, CH3CN and CH3OH. All these species appear to be concentrated towards the infrared-quiet methanol maser site G305A (G305.21+0.21). We suggest that this region contains an extremely deeply embedded site of massive star formation, with comparable qualities to the low-mass Class 0 stage. The infrared-bright methanol maser site G305B (G305.21+0.20) also exhibits emission in all the mapped transitions, but always at a lower level. We suggest this is because it harbours a site of massive star formation older and more developed than G305.21+0.21. All transitions appear to be extended beyond the size of the Mopra beam (30 arcsec). (CO)-C-13 and HCO+ line wings are suggestive of an outflow in the region, but the spatial resolution of these data is insufficient to identify the powering source. A narrow-lined (1.6 km s(-1) compared to a typical line FWHM of 6.4 km s(-1)) N2H+ source (G305SW) is found 90 arcsec to the south-west of the main star-forming centres, which does not correspond to any CH3CN or CH3OH source, nor does it correspond well to (CO)-C-13 or HCO+ emission in the vicinity. We suggest this may be a massive, cold, quiescent and possibly pre-stellar core. | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/1959.4/38531 | |
dc.language | English | |
dc.language.iso | EN | en_US |
dc.rights | CC BY-NC-ND 3.0 | en_US |
dc.rights.uri | https://creativecommons.org/licenses/by-nc-nd/3.0/au/ | en_US |
dc.source | Legacy MARC | en_US |
dc.subject.other | masers | en_US |
dc.subject.other | stars : formation | en_US |
dc.subject.other | ISM : molecules | en_US |
dc.subject.other | infrared : ISM | en_US |
dc.title | Mopra observations of G305.2+0.2: massive star formation at different evolutionary stages? | en_US |
dc.type | Journal Article | en |
dcterms.accessRights | metadata only access | |
dspace.entity.type | Publication | en_US |
unsw.accessRights.uri | http://purl.org/coar/access_right/c_14cb | |
unsw.description.notePublic | The Monthly Notices of the Royal Astronomical Society is published by Blackwell Publishing Ltd, http://www.blackwellpublishing.com/ | en_US |
unsw.identifier.doiPublisher | http://dx.doi.org/10.1111/j.1365-2966.2005.09711.x | en_US |
unsw.relation.faculty | Science | |
unsw.relation.ispartofissue | 1 | en_US |
unsw.relation.ispartofjournal | Monthly Notices of the Royal Astronomical Society | en_US |
unsw.relation.ispartofpagefrompageto | 321-326 | en_US |
unsw.relation.ispartofvolume | 365 | en_US |
unsw.relation.originalPublicationAffiliation | Walsh, Andrew, Physics, Faculty of Science, UNSW | en_US |
unsw.relation.originalPublicationAffiliation | Burton, Michael, Physics, Faculty of Science, UNSW | en_US |
unsw.relation.school | School of Physics | * |