Millimetric and submillimetric observations of IRAS 05327+3404 "holoea" in M36

O. Morata, Y. J. Kuan, P. T.P. Ho, H. C. Huang, E. A. Magnier, R. Zhao-Geisler

研究成果: 雜誌貢獻文章

摘要

The transition between the protostar, Class I, and the pre-main-sequence star, Class II, phases is still one of the most uncertain, and important, stages in the knowledge of the process of formation of an individual star because it is the stage that determines the final mass of the star. We observed the young stellar object "Holoea," associated with IRAS 05327+3404, which was classified as an object in the transition between the Class I and Class II phases with several unusual properties, and appears to be surrounded by large amounts of circumstellar material. We used the SMA and BIMA telescopes at millimeter and submillimeter (submm) wavelengths to observe the dust continuum emission and the CO (1-0) and (2-1), HCO+ (1-0) and (3-2), and HCN (1-0) transitions in the region around IRAS 05327+3404. We detected two continuum emission peaks at 1.1 mm: SMM 1, the submm counterpart of IRAS 05327+3404, and SMM 2, ∼6 arcsec to the west. The emissions of the three molecules show marked differences. The CO emission near the systemic velocity is filtered out by the telescopes, and CO mostly traces the high-velocity gas. The HCO+ and HCN emissions are more concentrated around the central parts of the region, and show several intensity peaks coincident with the submm continuum peaks. We identify two main molecular outflows: a bipolar outflow in an E-W direction that would be powered by SMM 1 and the other in a NE direction, which we associate with SMM 2. We propose that the SMM sources are probably Class I objects, with SMM 1 in an earlier evolutionary stage.

原文英語
文章編號49
期刊Astronomical Journal
146
發行號3
DOIs
出版狀態已發佈 - 2013 九月 1

指紋

Infrared Astronomy Satellite
continuums
outflow
telescopes
stars
spectral mixture analysis
pre-main sequence stars
protostars
dust
wavelength
gases
gas
wavelengths
molecules

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

引用此文

Millimetric and submillimetric observations of IRAS 05327+3404 "holoea" in M36. / Morata, O.; Kuan, Y. J.; Ho, P. T.P.; Huang, H. C.; Magnier, E. A.; Zhao-Geisler, R.

於: Astronomical Journal, 卷 146, 編號 3, 49, 01.09.2013.

研究成果: 雜誌貢獻文章

Morata, O. ; Kuan, Y. J. ; Ho, P. T.P. ; Huang, H. C. ; Magnier, E. A. ; Zhao-Geisler, R. / Millimetric and submillimetric observations of IRAS 05327+3404 "holoea" in M36. 於: Astronomical Journal. 2013 ; 卷 146, 編號 3.
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title = "Millimetric and submillimetric observations of IRAS 05327+3404 {"}holoea{"} in M36",
abstract = "The transition between the protostar, Class I, and the pre-main-sequence star, Class II, phases is still one of the most uncertain, and important, stages in the knowledge of the process of formation of an individual star because it is the stage that determines the final mass of the star. We observed the young stellar object {"}Holoea,{"} associated with IRAS 05327+3404, which was classified as an object in the transition between the Class I and Class II phases with several unusual properties, and appears to be surrounded by large amounts of circumstellar material. We used the SMA and BIMA telescopes at millimeter and submillimeter (submm) wavelengths to observe the dust continuum emission and the CO (1-0) and (2-1), HCO+ (1-0) and (3-2), and HCN (1-0) transitions in the region around IRAS 05327+3404. We detected two continuum emission peaks at 1.1 mm: SMM 1, the submm counterpart of IRAS 05327+3404, and SMM 2, ∼6 arcsec to the west. The emissions of the three molecules show marked differences. The CO emission near the systemic velocity is filtered out by the telescopes, and CO mostly traces the high-velocity gas. The HCO+ and HCN emissions are more concentrated around the central parts of the region, and show several intensity peaks coincident with the submm continuum peaks. We identify two main molecular outflows: a bipolar outflow in an E-W direction that would be powered by SMM 1 and the other in a NE direction, which we associate with SMM 2. We propose that the SMM sources are probably Class I objects, with SMM 1 in an earlier evolutionary stage.",
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AU - Morata, O.

AU - Kuan, Y. J.

AU - Ho, P. T.P.

AU - Huang, H. C.

AU - Magnier, E. A.

AU - Zhao-Geisler, R.

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AB - The transition between the protostar, Class I, and the pre-main-sequence star, Class II, phases is still one of the most uncertain, and important, stages in the knowledge of the process of formation of an individual star because it is the stage that determines the final mass of the star. We observed the young stellar object "Holoea," associated with IRAS 05327+3404, which was classified as an object in the transition between the Class I and Class II phases with several unusual properties, and appears to be surrounded by large amounts of circumstellar material. We used the SMA and BIMA telescopes at millimeter and submillimeter (submm) wavelengths to observe the dust continuum emission and the CO (1-0) and (2-1), HCO+ (1-0) and (3-2), and HCN (1-0) transitions in the region around IRAS 05327+3404. We detected two continuum emission peaks at 1.1 mm: SMM 1, the submm counterpart of IRAS 05327+3404, and SMM 2, ∼6 arcsec to the west. The emissions of the three molecules show marked differences. The CO emission near the systemic velocity is filtered out by the telescopes, and CO mostly traces the high-velocity gas. The HCO+ and HCN emissions are more concentrated around the central parts of the region, and show several intensity peaks coincident with the submm continuum peaks. We identify two main molecular outflows: a bipolar outflow in an E-W direction that would be powered by SMM 1 and the other in a NE direction, which we associate with SMM 2. We propose that the SMM sources are probably Class I objects, with SMM 1 in an earlier evolutionary stage.

KW - ISM: clouds

KW - ISM: individual objects (IRAS 05327+3404)

KW - ISM: jets and outflows

KW - ISM: molecules

KW - stars: protostars

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