Publication:
Radio observations of comet 9P/Tempel 1 with the Australia Telescope facilities during the Deep Impact encounter
Radio observations of comet 9P/Tempel 1 with the Australia Telescope facilities during the Deep Impact encounter
dc.contributor.author | Jones, P. A. | en_US |
dc.contributor.author | Sarkissian, J. M. | en_US |
dc.contributor.author | Burton, Michael | en_US |
dc.contributor.author | Voronkov, M. A. | en_US |
dc.contributor.author | Filipovic, M. D. | en_US |
dc.date.accessioned | 2021-11-25T12:55:41Z | |
dc.date.available | 2021-11-25T12:55:41Z | |
dc.date.issued | 2006 | en_US |
dc.description.abstract | We present radio observations of comet 9P/Tempel 1 associated with the Deep Impact spacecraft collision of 2005 July 4. Weak 18-cm OH emission was detected with the Parkes 64-m telescope, in data averaged over July 4-6, at a level of 12 +/- 3 mJy km s(-1), corresponding to OH production rate 2.8 x 10(28) molecules s(-1) ( Despois et al. inversion model, or 1.0 x 10(28) s(-1) for the Schleicher & A`Hearn model). We did not detect the HCN 1-0 line with the Mopra 22-m telescope over the period July 2-6. The 3 sigma limit of 0.06K kms(-1) for HCN on July 4 after the impact gives the limit to the HCN production rate of < 1.8 x 10(25) s(-1). We did not detect the HCN 1-0 line, 6.7 GHz CH3OH line or 3.4-mm continuum with the Australia Telescope Compact Array (ATCA) on July 4, giving further limits on any small-scale structure due to an outburst. The 3 sigma limit on HCN emission of 2.5Kkms(-1) from the ATCA around impact corresponds to limit < 4 x 10(29) HCN molecules released by the impact. | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/1959.4/38573 | |
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 | comets : individual | en_US |
dc.subject.other | 9P/Tempel 1 | en_US |
dc.subject.other | radio lines : Solar system | en_US |
dc.title | Radio observations of comet 9P/Tempel 1 with the Australia Telescope facilities during the Deep Impact encounter | en_US |
dc.type | Journal Article | en |
dcterms.accessRights | open access | |
dspace.entity.type | Publication | en_US |
unsw.accessRights.uri | https://purl.org/coar/access_right/c_abf2 | |
unsw.description.notePublic | The definitive version is available at www.blackwell-synergy.com | en_US |
unsw.identifier.doiPublisher | http://dx.doi.org/10.1111/j.1365-2966.2006.10460.x | en_US |
unsw.relation.faculty | Science | |
unsw.relation.ispartofissue | 4 | en_US |
unsw.relation.ispartofjournal | Monthly Notices of the Royal Astronomical Society | en_US |
unsw.relation.ispartofpagefrompageto | 1995-2000 | en_US |
unsw.relation.ispartofvolume | 369 | en_US |
unsw.relation.originalPublicationAffiliation | Jones, P. A. , Australia Telescope National Facility | en_US |
unsw.relation.originalPublicationAffiliation | Sarkissian, J. M. , Australia Telescope Facility | en_US |
unsw.relation.originalPublicationAffiliation | Burton, Michael, Physics, Faculty of Science, UNSW | en_US |
unsw.relation.originalPublicationAffiliation | Voronkov, M. A. , Australia Telescope Facility | en_US |
unsw.relation.originalPublicationAffiliation | Filipovic, M. D. , University of Western Sydney | en_US |
unsw.relation.school | School of Physics | * |
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