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- Publisher Website: 10.1046/j.1365-8711.2002.05777.x
- Scopus: eid_2-s2.0-0041702408
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Article: Mid-infrared, Hα and radio continuum images of an unusual H II region, G308.70 + 0.60
Title | Mid-infrared, Hα and radio continuum images of an unusual H II region, G308.70 + 0.60 |
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Authors | |
Keywords | Radio continuum: ISM H II regions Infrared: ISM Infrared: stars ISM: structure Stars: formation |
Issue Date | 2002 |
Citation | Monthly Notices of the Royal Astronomical Society, 2002, v. 336, n. 3, p. 736-746 How to Cite? |
Abstract | We report on a multi-wavelength study of images in the mid-infrared (MIR), Hα and radio continuum of an unusual H II region, G308.70 + 0.60. Using images from the Midcourse Space Experiment (MSX) between 8.3 and 21.3 μm, from the AAO/UK Schmidt Telescope (UKST) deep, high-resolution, Hα survey of the plane, and from the Molonglo Observatory Synthesis Telescope (MOST) Galactic plane survey in the radio continuum at 843 MHz, we have investigated the morphology of the nebula and propose that there is an interaction between the interstellar medium and a star lying inside the large nebular bubble. Secondary star formation appears to have occurred in several places on the dense rim of the bubble. In one such site, this has resulted in a luminous MIR double star, situated within the rim of the nebular ring, that has created its own local bubble. |
Persistent Identifier | http://hdl.handle.net/10722/208822 |
ISSN | 2023 Impact Factor: 4.7 2023 SCImago Journal Rankings: 1.621 |
ISI Accession Number ID |
DC Field | Value | Language |
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dc.contributor.author | Cohen, Martin G. | - |
dc.contributor.author | Green, Anne J. | - |
dc.contributor.author | Parker, Quentin A. | - |
dc.contributor.author | Mader, Stacy L. | - |
dc.contributor.author | Cannon, Russell D. | - |
dc.date.accessioned | 2015-03-23T02:01:49Z | - |
dc.date.available | 2015-03-23T02:01:49Z | - |
dc.date.issued | 2002 | - |
dc.identifier.citation | Monthly Notices of the Royal Astronomical Society, 2002, v. 336, n. 3, p. 736-746 | - |
dc.identifier.issn | 0035-8711 | - |
dc.identifier.uri | http://hdl.handle.net/10722/208822 | - |
dc.description.abstract | We report on a multi-wavelength study of images in the mid-infrared (MIR), Hα and radio continuum of an unusual H II region, G308.70 + 0.60. Using images from the Midcourse Space Experiment (MSX) between 8.3 and 21.3 μm, from the AAO/UK Schmidt Telescope (UKST) deep, high-resolution, Hα survey of the plane, and from the Molonglo Observatory Synthesis Telescope (MOST) Galactic plane survey in the radio continuum at 843 MHz, we have investigated the morphology of the nebula and propose that there is an interaction between the interstellar medium and a star lying inside the large nebular bubble. Secondary star formation appears to have occurred in several places on the dense rim of the bubble. In one such site, this has resulted in a luminous MIR double star, situated within the rim of the nebular ring, that has created its own local bubble. | - |
dc.language | eng | - |
dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society | - |
dc.subject | Radio continuum: ISM | - |
dc.subject | H II regions | - |
dc.subject | Infrared: ISM | - |
dc.subject | Infrared: stars | - |
dc.subject | ISM: structure | - |
dc.subject | Stars: formation | - |
dc.title | Mid-infrared, Hα and radio continuum images of an unusual H II region, G308.70 + 0.60 | - |
dc.type | Article | - |
dc.description.nature | link_to_OA_fulltext | - |
dc.identifier.doi | 10.1046/j.1365-8711.2002.05777.x | - |
dc.identifier.scopus | eid_2-s2.0-0041702408 | - |
dc.identifier.volume | 336 | - |
dc.identifier.issue | 3 | - |
dc.identifier.spage | 736 | - |
dc.identifier.epage | 746 | - |
dc.identifier.isi | WOS:000178860300008 | - |
dc.identifier.issnl | 0035-8711 | - |