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Investigating the role of magnetic fields in star formation using molecular line profiles

Research output: Contribution to journalArticlepeer-review

Author(s)

Charles Yin, Felix D Priestley, James Wurster

School/Research organisations

Abstract

Determining the importance of magnetic fields in star-forming environments is hampered by the difficulty of accurately measuring both field strength and gas properties in molecular clouds. We post-process three-dimensional non-ideal magnetohydrodynamic simulations of pre-stellar cores with a time-dependent chemical network, and use radiative transfer modelling to calculate self-consistent molecular line profiles. Varying the initial mass-to-flux ratio from subcritical to supercritical results in significant changes to both the intensity and shape of several observationally important molecular lines. We identify the peak intensity ratio of N2H+ to CS lines, and the CS J = 2–1 blue-to-red peak intensity ratio, as promising diagnostics of the initial mass-to-flux ratio, with N2H+/CS values of >0.6 (<0.2) and CS blue/red values of <3 (>5) indicating subcritical (supercritical) collapse. These criteria suggest that, despite presently being magnetically supercritical, L1498 formed from subcritical initial conditions.

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Details

Original languageEnglish
Pages (from-to)2381–2389
JournalMonthly Notices of the Royal Astronomical Society
Volume504
Issue number2
Early online date20 Apr 2021
DOIs
Publication statusPublished - Jun 2021

    Research areas

  • Astrochemistry, MHD, Stars: formation, ISM: magnetic fields, ISM: molecules

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