dc.contributor.author | Chené, A. -N. | |
dc.contributor.author | Benjamin, R. A. | |
dc.contributor.author | Alegría, S. Ramírez | |
dc.contributor.author | Borissova, J. | |
dc.contributor.author | Kurtev, R. | |
dc.contributor.author | Bidin, C. Moni | |
dc.contributor.author | Mauro, F. | |
dc.contributor.author | Lucas, P. | |
dc.contributor.author | Guo, Z. | |
dc.contributor.author | Smith, L. C. | |
dc.contributor.author | Gonzalez-Fernandez, C. | |
dc.contributor.author | Ivanov, V. D. | |
dc.contributor.author | Minniti, D. | |
dc.contributor.author | Anderson, L. D. | |
dc.contributor.author | Armentrout, W. P. | |
dc.contributor.author | Gonzalez, D. | |
dc.contributor.author | Herrero, A. | |
dc.contributor.author | Ramírez, K. Peña | |
dc.date.accessioned | 2021-06-18T15:00:01Z | |
dc.date.available | 2021-06-18T15:00:01Z | |
dc.date.issued | 2021-04-20 | |
dc.identifier.citation | Chené , A -N , Benjamin , R A , Alegría , S R , Borissova , J , Kurtev , R , Bidin , C M , Mauro , F , Lucas , P , Guo , Z , Smith , L C , Gonzalez-Fernandez , C , Ivanov , V D , Minniti , D , Anderson , L D , Armentrout , W P , Gonzalez , D , Herrero , A & Ramírez , K P 2021 , ' Assessing the stellar population and the environment of an HII region on the far side of the Galaxy ' , The Astrophysical Journal , vol. 911 , no. 2 , 91 . https://doi.org/10.3847/1538-4357/abec6f | |
dc.identifier.issn | 0004-637X | |
dc.identifier.other | ArXiv: http://arxiv.org/abs/2103.05849v1 | |
dc.identifier.other | ORCID: /0000-0002-8872-4462/work/95730886 | |
dc.identifier.uri | http://hdl.handle.net/2299/24591 | |
dc.description | © 2021. The American Astronomical Society. All rights reserved. This is the accepted manuscript version of an article which has been published in final form at https://doi.org/10.3847/1538-4357/abec6f | |
dc.description.abstract | We have investigated the stellar and interstellar content of the distant star formation region IRAS 17591-2228 (WISE HII region GAL 007.47+0.06). It is associated to a water maser, whose parallax distance is d=20.4^{+2.8} {-2.2} kpc, supported by independent measurements of proper motion and radial velocity. It is projected in the same direction as an extremely red (J-Ks ~ 6 mag) group of stars, and a shell of mid-infrared emission. We qualify the group of stars as a cluster candidate, VVV CL177. Its radius spans between 0.45' and 1' and contains at least two young stellar objects with an extreme extinction near Av ~ 40 mag. Yet more analysis will be required to determine is it is a real single cluster associated with the water maser. The 13CO emissions at the radial velocity of the maser corresponds to the mid-infrared emission. | en |
dc.format.extent | 8 | |
dc.format.extent | 601531 | |
dc.language.iso | eng | |
dc.relation.ispartof | The Astrophysical Journal | |
dc.subject | astro-ph.GA | |
dc.subject | astro-ph.SR | |
dc.title | Assessing the stellar population and the environment of an HII region on the far side of the Galaxy | en |
dc.contributor.institution | Centre for Astrophysics Research | |
dc.contributor.institution | Centre for Climate Change Research (C3R) | |
dc.contributor.institution | School of Physics, Engineering & Computer Science | |
dc.contributor.institution | Department of Physics, Astronomy and Mathematics | |
dc.contributor.institution | School of Physics, Astronomy and Mathematics | |
dc.description.status | Peer reviewed | |
dc.date.embargoedUntil | 2022-04-20 | |
rioxxterms.versionofrecord | 10.3847/1538-4357/abec6f | |
rioxxterms.type | Journal Article/Review | |
herts.preservation.rarelyaccessed | true | |