Facial reconstruction

Search LJMU Research Online

Browse Repository | Browse E-Theses

Star formation in 'the Brick': ALMA reveals an active proto-cluster in the Galactic centre cloud G0.253+0.016

Walker, DL, Longmore, SN, Bally, J, Ginsburg, A, Kruijssen, JMD, Zhang, Q, Henshaw, JD, Lu, X, Alves, J, Barnes, AT, Battersby, C, Beuther, H, Contreras, YA, Gómez, L, Ho, LC, Jackson, JM, Kauffmann, J, Mills, EAC and Pillai, T Star formation in 'the Brick': ALMA reveals an active proto-cluster in the Galactic centre cloud G0.253+0.016. Monthly Notices of the Royal Astronomical Society. ISSN 0035-8711 (Accepted)

[img]
Preview
Text
2102.03560v1.pdf - Accepted Version

Download (10MB) | Preview

Abstract

G0.253+0.016, aka 'the Brick', is one of the most massive (> 10^5 Msun) and dense (> 10^4 cm-3) molecular clouds in the Milky Way's Central Molecular Zone. Previous observations have detected tentative signs of active star formation, most notably a water maser that is associated with a dust continuum source. We present ALMA Band 6 observations with an angular resolution of 0.13" (1000 AU) towards this 'maser core', and report unambiguous evidence of active star formation within G0.253+0.016. We detect a population of eighteen continuum sources (median mass ~ 2 Msun), nine of which are driving bi-polar molecular outflows as seen via SiO (5-4) emission. At the location of the water maser, we find evidence for a protostellar binary/multiple with multi-directional outflow emission. Despite the high density of G0.253+0.016, we find no evidence for high-mass protostars in our ALMA field. The observed sources are instead consistent with a cluster of low-to-intermediate-mass protostars. However, the measured outflow properties are consistent with those expected for intermediate-to-high-mass star formation. We conclude that the sources are young and rapidly accreting, and may potentially form intermediate and high-mass stars in the future. The masses and projected spatial distribution of the cores are generally consistent with thermal fragmentation, suggesting that the large-scale turbulence and strong magnetic field in the cloud do not dominate on these scales, and that star formation on the scale of individual protostars is similar to that in Galactic disc environments.

Item Type: Article
Additional Information: This is a pre-copyedited, author-produced PDF of an article accepted for publication in Monthly Notices of the Royal Astronomical Society following peer review. The version of record Daniel L Walker, Steven N Longmore, John Bally, Adam Ginsburg, J M Diederik Kruijssen, Qizhou Zhang, Jonathan D Henshaw, Xing Lu, João Alves, Ashley T Barnes, Cara Battersby, Henrik Beuther, Yanett A Contreras, Laura Gómez, Luis C Ho, James M Jackson, Jens Kauffmann, Elisabeth A C Mills, Thushara Pillai, Star formation in ‘the Brick’: ALMA reveals an active proto-cluster in the Galactic centre cloud G0.253+0.016, Monthly Notices of the Royal Astronomical Society, 2021;, stab415, is available online at: https://doi.org/10.1093/mnras/stab415
Uncontrolled Keywords: astro-ph.GA; astro-ph.GA
Subjects: Q Science > QB Astronomy
Q Science > QC Physics
Divisions: Astrophysics Research Institute
Publisher: Oxford University Press
Related URLs:
Date Deposited: 15 Feb 2021 12:12
Last Modified: 15 Feb 2021 12:15
DOI or Identification number: 10.1093/mnras/stab415
URI: https://researchonline.ljmu.ac.uk/id/eprint/14460

Actions (login required)

View Item View Item