The momentum budget of clustered supernova feedback in a 3D, magnetized medium

While the evolution of superbubbles driven by clustered supernovae has been studied by numerous authors, the resulting radial momentum yield is uncertain by as much as an order of magnitude depending on the computational methods and assumed properties of the surrounding interstellar medium (ISM). In...

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Published in:Monthly notices of the Royal Astronomical Society Vol. 483; no. 3; pp. 3647 - 3658
Main Authors: Gentry, Eric S, Krumholz, Mark R, Madau, Piero, Lupi, Alessandro
Format: Journal Article
Language:English
Published: Oxford University Press (OUP): Policy P - Oxford Open Option A 01.03.2019
Subjects:
Astrophysics
Sciences of the Universe
Astrophysics - Astrophysics of Galaxies
ISM: supernova remnants
hydrodynamics
magnetic fields
ISM: bubbles
ISSN:0035-8711, 1365-2966
Online Access:Get full text
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Abstract While the evolution of superbubbles driven by clustered supernovae has been studied by numerous authors, the resulting radial momentum yield is uncertain by as much as an order of magnitude depending on the computational methods and assumed properties of the surrounding interstellar medium (ISM). In this work, we study the origin of these discrepancies, and seek to determine the correct momentum budget for a homogeneous ISM. We carry out 3D hydrodynamic and magnetohydrodynamic (MHD) simulations of clustered supernova explosions, using a Lagrangian method and checking for convergence with respect to resolution. We find that the terminal momentum of a shell driven by clustered supernovae is dictated primarily by the mixing rate across the contact discontinuity between the hot and cold phases, and that this energy mixing rate is dominated by numerical diffusion even at the highest resolution we can complete, 0.03 M⊙. Magnetic fields also reduce the mixing rate, so that MHD simulations produce higher momentum yields than HD ones at equal resolution. As a result, we obtain only a lower limit on the momentum yield from clustered supernovae. Combining this with our previous 1D results, which provide an upper limit because they allow almost no mixing across the contact discontinuity, we conclude that the momentum yield per supernova from clustered supernovae in a homogeneous ISM is bounded between 2 × 105 and 3 × 106 M⊙ km s-1. A converged value for the simple homogeneous ISM remains elusive.
AbstractList While the evolution of superbubbles driven by clustered supernovae has been studied by numerous authors, the resulting radial momentum yield is uncertain by as much as an order of magnitude depending on the computational methods and assumed properties of the surrounding interstellar medium (ISM). In this work, we study the origin of these discrepancies, and seek to determine the correct momentum budget for a homogeneous ISM. We carry out 3D hydrodynamic and magnetohydrodynamic (MHD) simulations of clustered supernova explosions, using a Lagrangian method and checking for convergence with respect to resolution. We find that the terminal momentum of a shell driven by clustered supernovae is dictated primarily by the mixing rate across the contact discontinuity between the hot and cold phases, and that this energy mixing rate is dominated by numerical diffusion even at the highest resolution we can complete, 0.03 M⊙. Magnetic fields also reduce the mixing rate, so that MHD simulations produce higher momentum yields than HD ones at equal resolution. As a result, we obtain only a lower limit on the momentum yield from clustered supernovae. Combining this with our previous 1D results, which provide an upper limit because they allow almost no mixing across the contact discontinuity, we conclude that the momentum yield per supernova from clustered supernovae in a homogeneous ISM is bounded between 2 × 105 and 3 × 106 M⊙ km s-1. A converged value for the simple homogeneous ISM remains elusive.
Author Gentry, Eric S
Lupi, Alessandro
Krumholz, Mark R
Madau, Piero
Author_xml – sequence: 1
  givenname: Eric S
  orcidid: 0000-0002-4906-3745
  surname: Gentry
  fullname: Gentry, Eric S
  organization: Department of Astronomy and Astrophysics, University of California at Santa Cruz, 1156 High St, Santa Cruz, CA 95064, USA
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  givenname: Mark R
  orcidid: 0000-0003-3893-854X
  surname: Krumholz
  fullname: Krumholz, Mark R
  organization: Research School of Astronomy, Astrophysics, Australian National University, Canberra, ACT 2611, Australia
– sequence: 3
  givenname: Piero
  surname: Madau
  fullname: Madau, Piero
  organization: Department of Astronomy and Astrophysics, University of California at Santa Cruz, 1156 High St, Santa Cruz, CA 95064, USA, Sorbonne Université, CNRS, UMR 7095, Institut d’Astrophysique de Paris, 98 bis bd Arago, F-75014 Paris, France
– sequence: 4
  givenname: Alessandro
  orcidid: 0000-0001-6106-7821
  surname: Lupi
  fullname: Lupi, Alessandro
  organization: Scuola Normale Superiore, Piazza dei Cavalieri 7, I-56126 Pisa, Italy
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Issue 3
Keywords Astrophysics - Astrophysics of Galaxies
ISM: supernova remnants
hydrodynamics
magnetic fields
ISM: bubbles
Language English
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SubjectTerms Astrophysics
Sciences of the Universe
Title The momentum budget of clustered supernova feedback in a 3D, magnetized medium
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