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The Effect of Molecular Cloud Properties on the Kinematics of Stars Formed in the Trifid Region

Kuhn, Michael A. and Hillenbrand, Lynne A. and Feigelson, Eric D. and Fowler, Ian and Getman, Konstantin V. and Broos, Patrick S. and Povich, Matthew S. and Gromadzki, Mariusz (2022) The Effect of Molecular Cloud Properties on the Kinematics of Stars Formed in the Trifid Region. Astrophysical Journal, 937 (1). Art. No. 46. ISSN 0004-637X. doi:10.3847/1538-4357/ac6fe8.

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The dynamical states of molecular clouds may affect the properties of the stars they form. In the vicinity of the Trifid Nebula (d = 1180 ± 25 pc), the main star cluster (Trifid Main) lies within an expanding section of the molecular cloud; however, ∼0.°3 to the north (Trifid North), the cloud’s velocity structure is more tranquil. We acquired a Chandra X-ray observation to identify pre-main-sequence stars in Trifid North, complementing a previous observation of Trifid Main. In Trifid North, we identified 51 candidate pre-main-sequence stars, of which 13 are high-confidence Trifid members based on Gaia EDR3 parallaxes and proper motions. We also reanalyzed the membership of Trifid Main and separated out multiple background stellar associations. Trifid North represents a stellar population ∼10% as rich as Trifid Main that formed in a separate part of the cloud. The 1D stellar velocity dispersion in Trifid North (0.6 ± 0.2 km s⁻¹) is 3 times lower than that in Trifid Main (1.9 ± 0.2 km s⁻¹). Furthermore, in Trifid Main, proper motions indicate that the portion of the star cluster superimposed on the optical nebula is expanding. Expansion of the H ii region around the O-star HD 164492A, and the resulting gas expulsion, can explain both the motions of the stars and gas in Trifid Main. Contrary to previous studies, we find no evidence that a cloud–cloud collision triggered star formation in the region.

Item Type:Article
Related URLs:
URLURL TypeDescription ItemDiscussion paper
Kuhn, Michael A.0000-0002-0631-7514
Feigelson, Eric D.0000-0002-5077-6734
Fowler, Ian0000-0002-4958-8648
Getman, Konstantin V.0000-0002-6137-8280
Broos, Patrick S.0000-0002-7872-2025
Povich, Matthew S.0000-0001-9062-3583
Gromadzki, Mariusz0000-0002-1650-1518
Additional Information:This research was supported by Chandra grant GO9-20002X. This work is based on data from ESAs Gaia mission (Gaia Collaboration et al. 2016), processed by the Data Processing and Analysis Consortium, funded by national institutions, particularly those participating in the Gaia Multilateral Agreement. We thank David James and Sean Points for assistance with ARCoIRIS, Katelyn Allers for the modified Spextool software, Paul Crowther and Philip Massey for suggestions about spectral classification, and the anonymous referee for useful comments. I.E.F. was supported by Caltechs Freshman Summer Research Institute (FSRI). M.G. is supported by the EU Horizon 2020 research and innovation program under grant agreement No. 101004719.
Group:Astronomy Department
Funding AgencyGrant Number
NASA ChandraGO9-20002X
Gaia Multilateral AgreementUNSPECIFIED
Caltech Freshman Summer Research Institute (FSRI)UNSPECIFIED
European Research Council (ERC)101004719
Issue or Number:1
Record Number:CaltechAUTHORS:20221013-48351800.3
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Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:117395
Deposited By: Research Services Depository
Deposited On:14 Oct 2022 22:31
Last Modified:14 Oct 2022 22:36

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