TY - JOUR
T1 - First extragalactic measurement of the turbulence driving parameter
T2 - ALMA observations of the star-foing region N159E in the Large Magellanic Cloud
AU - Sharda, Piyush
AU - Menon, Shyam H.
AU - Federrath, Christoph
AU - Krumholz, Mark R.
AU - Beattie, James R.
AU - Jameson, Katherine E.
AU - Tokuda, Kazuki
AU - Burkhart, Blakesley
AU - Crocker, Roland M.
AU - Law, Charles J.
AU - Seta, Amit
AU - Gaetz, Terrance J.
AU - Pingel, Nickolas M.
AU - Seitenzahl, Ivo R.
AU - Sano, Hidetoshi
AU - Fukui, Yasuo
N1 - Publisher Copyright:
© 2021 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society.
PY - 2022/1/1
Y1 - 2022/1/1
N2 - Studying the driving modes of turbulence is important for characterizing the impact of turbulence in various astrophysical environments. The driving mode of turbulence is parametrized by b, which relates the width of the gas density PDF to the turbulent Mach number; b ≈ 1/3, 1, and 0.4 correspond to driving that is solenoidal, compressive, and a natural mixture of the two, respectively. In this work, we use high-resolution (sub-pc) ALMA 12CO (J = 2-1), 13CO (J = 2-1), and C18O (J = 2-1) observations of filamentary molecular clouds in the star-foing region N159E (the Papillon Nebula) in the Large Magellanic Cloud (LMC) to provide the first measurement of turbulence driving parameter in an extragalactic region. We use a non-local theodynamic equilibrium (NLTE) analysis of the CO isotopologues to construct a gas density PDF, which we find to be largely lognoal in shape with some inteittent features indicating deviations from lognoality. We find that the width of the lognoal part of the density PDF is comparable to the supersonic turbulent Mach number, resulting in b ≈ 0.9. This implies that the driving mode of turbulence in N159E is primarily compressive. We speculate that the compressive turbulence could have been powered by gravo-turbulent fragmentation of the molecular gas, or due to compression powered by H i flows that led to the development of the molecular filaments observed by ALMA in the region. Our analysis can be easily applied to study the nature of turbulence driving in resolved star-foing regions in the local as well as the high-redshift Universe.
AB - Studying the driving modes of turbulence is important for characterizing the impact of turbulence in various astrophysical environments. The driving mode of turbulence is parametrized by b, which relates the width of the gas density PDF to the turbulent Mach number; b ≈ 1/3, 1, and 0.4 correspond to driving that is solenoidal, compressive, and a natural mixture of the two, respectively. In this work, we use high-resolution (sub-pc) ALMA 12CO (J = 2-1), 13CO (J = 2-1), and C18O (J = 2-1) observations of filamentary molecular clouds in the star-foing region N159E (the Papillon Nebula) in the Large Magellanic Cloud (LMC) to provide the first measurement of turbulence driving parameter in an extragalactic region. We use a non-local theodynamic equilibrium (NLTE) analysis of the CO isotopologues to construct a gas density PDF, which we find to be largely lognoal in shape with some inteittent features indicating deviations from lognoality. We find that the width of the lognoal part of the density PDF is comparable to the supersonic turbulent Mach number, resulting in b ≈ 0.9. This implies that the driving mode of turbulence in N159E is primarily compressive. We speculate that the compressive turbulence could have been powered by gravo-turbulent fragmentation of the molecular gas, or due to compression powered by H i flows that led to the development of the molecular filaments observed by ALMA in the region. Our analysis can be easily applied to study the nature of turbulence driving in resolved star-foing regions in the local as well as the high-redshift Universe.
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U2 - 10.1093/mnras/stab3048
DO - 10.1093/mnras/stab3048
M3 - Article
AN - SCOPUS:85121264938
VL - 509
SP - 2180
EP - 2193
JO - Monthly Notices of the Royal Astronomical Society
JF - Monthly Notices of the Royal Astronomical Society
SN - 0035-8711
IS - 2
ER -