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A necklace of dense cores in the high-mass star forming region G35.20−0.74 N: ALMA observations

Sánchez-Monge, Á. and Beltrán, M. T. and Cesaroni, R. and Etoka, S. and Galli, D. and Kumar, M. S. N. and Moscadelli, L. and Stanke, T. and van der Tak, F. F. S. and Vig, S. and Walmsley, C. M. and Wang, K.-S. and Zinnecker, H. and Elia, D. and Molinari, S. and Schisano, E. (2014) A necklace of dense cores in the high-mass star forming region G35.20−0.74 N: ALMA observations. Astronomy and Astrophysics, 569 . Art. No. A11. ISSN 0004-6361. https://resolver.caltech.edu/CaltechAUTHORS:20141124-075933786

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Abstract

Context. The formation process of high-mass stars (with masses >8 M_⊙) is still poorly understood, and represents a challenge from both the theoretical and observational points of view. The advent of the Atacama Large Millimeter Array (ALMA) is expected to provide observational evidence to better constrain the theoretical scenarios. Aims. The present study aims at characterizing the high-mass star forming region G35.20−0.74 N, which is found associated with at least one massive outflow and contains multiple dense cores, one of them recently found associated with a Keplerian rotating disk. Methods. We used the radio-interferometer ALMA to observe the G35.20−0.74 N region in the submillimeter continuum and line emission at 350 GHz. The observed frequency range covers tracers of dense gas (e.g., H^(13)CO^+, C^(17)O), molecular outflows (e.g., SiO), and hot cores (e.g., CH_3CN, CH_3OH). These observations were complemented with infrared and centimeter data. Results. The ALMA 870 μm continuum emission map reveals an elongated dust structure (~0.15 pc long and ~0.013 pc wide; full width at half maximum) perpendicular to the large-scale molecular outflow detected in the region, and fragmented into a number of cores with masses ~1–10 M_⊙ and sizes ~1600 AU (spatial resolution ~960 AU). The cores appear regularly spaced with a separation of ~0.023 pc. The emission of dense gas tracers such as H^(13)CO^+ or C^(17)O is extended and coincident with the dust elongated structure. The three strongest dust cores show emission of complex organic molecules characteristic of hot cores, with temperatures around 200 K, and relative abundances 0.2–2 × 10^(-8) for CH_3CN and 0.6–5 × 10^(-6) for CH_3OH. The two cores with highest mass (cores A and B) show coherent velocity fields, with gradients almost aligned with the dust elongated structure. Those velocity gradients are consistent with Keplerian disks rotating about central masses of 4–18 M_⊙. Perpendicular to the velocity gradients we have identified a large-scale precessing jet/outflow associated with core B, and hints of an east-west jet/outflow associated with core A. Conclusions. The elongated dust structure in G35.20−0.74 N is fragmented into a number of dense cores that may form high-mass stars. Based on the velocity field of the dense gas, the orientation of the magnetic field, and the regularly spaced fragmentation, we interpret this elongated structure as the densest part of a 1D filament fragmenting and forming high-mass stars.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://www.aanda.org/articles/aa/abs/2014/09/aa24032-14/aa24032-14.htmlPublisherArticle
http://dx.doi.org/10.1051/0004-6361/201424032DOIArticle
http://arxiv.org/abs/1406.4081arXivArticle
Additional Information:© 2014 ESO. Article published by EDP Sciences. Received 18 April 2014. Accepted 9 June 2014. Published online 09 September 2014. We are grateful to the Italian ARC node for the usage of their computer facilities during the cleaning and imaging process. We are also grateful to Ray Furuya for providing us the ASTE spectrum, and to Keping Qiu for providing the SMA spectra. Á.S.-M. is grateful to Peter Schilke, Thomas Möller and Alexander Zernickel for helping with the analysis of the my XCLASS software. This paper makes use of the following ALMA data: ADS/JAO.ALMA#2011.0.00275.S. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada) and NSC and ASIAA (Taiwan), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ. This publication makes use of data products from the Widefield Infrared Survey Explorer, which is a joint project of the University of California, Los Angeles, and the Jet Propulsion Laboratory/California Institute of Technology, funded by the National Aeronautics and Space Administration.
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NASAUNSPECIFIED
Subject Keywords:stars: formation, stars: massive, ISM: individual objects: G35.20–0.74 N, ISM: molecules, ISM: jets and outflows
Record Number:CaltechAUTHORS:20141124-075933786
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20141124-075933786
Official Citation:A necklace of dense cores in the high-mass star forming region G35.20−0.74 N: ALMA observations A11 Á. Sánchez-Monge, M. T. Beltrán, R. Cesaroni, S. Etoka, D. Galli, M. S. N. Kumar, L. Moscadelli, T. Stanke, F. F. S. van der Tak, S. Vig, et al. (6 more) Published online: 9 September 2014 DOI: http://dx.doi.org/10.1051/0004-6361/201424032
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:52079
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:24 Nov 2014 17:26
Last Modified:03 Oct 2019 07:39

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