Chemical solver to compute molecule and grain abundances and non-ideal MHD resistivities in prestellar core-collapse calculations ?

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Standard

Chemical solver to compute molecule and grain abundances and non-ideal MHD resistivities in prestellar core-collapse calculations ? / Marchand, P.; Masson, J.; Chabrier, G.; Hennebelle, P.; Commercon, B.; Vaytet, N.

I: Astronomy & Astrophysics, Bind 592, A18, 08.2016.

Publikation: Bidrag til tidsskriftTidsskriftartikelForskningfagfællebedømt

Harvard

Marchand, P, Masson, J, Chabrier, G, Hennebelle, P, Commercon, B & Vaytet, N 2016, 'Chemical solver to compute molecule and grain abundances and non-ideal MHD resistivities in prestellar core-collapse calculations ?', Astronomy & Astrophysics, bind 592, A18. https://doi.org/10.1051/0004-6361/201526780

APA

Marchand, P., Masson, J., Chabrier, G., Hennebelle, P., Commercon, B., & Vaytet, N. (2016). Chemical solver to compute molecule and grain abundances and non-ideal MHD resistivities in prestellar core-collapse calculations ? Astronomy & Astrophysics, 592, [A18]. https://doi.org/10.1051/0004-6361/201526780

Vancouver

Marchand P, Masson J, Chabrier G, Hennebelle P, Commercon B, Vaytet N. Chemical solver to compute molecule and grain abundances and non-ideal MHD resistivities in prestellar core-collapse calculations ? Astronomy & Astrophysics. 2016 aug.;592. A18. https://doi.org/10.1051/0004-6361/201526780

Author

Marchand, P. ; Masson, J. ; Chabrier, G. ; Hennebelle, P. ; Commercon, B. ; Vaytet, N. / Chemical solver to compute molecule and grain abundances and non-ideal MHD resistivities in prestellar core-collapse calculations ?. I: Astronomy & Astrophysics. 2016 ; Bind 592.

Bibtex

@article{1b0a334d68e2488287203469b3e85e90,
title = "Chemical solver to compute molecule and grain abundances and non-ideal MHD resistivities in prestellar core-collapse calculations ?",
keywords = "magnetohydrodynamics (MHD), ISM: molecules, stars: formation",
author = "P. Marchand and J. Masson and G. Chabrier and P. Hennebelle and B. Commercon and N. Vaytet",
year = "2016",
month = aug,
doi = "10.1051/0004-6361/201526780",
language = "English",
volume = "592",
journal = "Astronomy & Astrophysics",
issn = "0004-6361",
publisher = "E D P Sciences",

}

RIS

TY - JOUR

T1 - Chemical solver to compute molecule and grain abundances and non-ideal MHD resistivities in prestellar core-collapse calculations ?

AU - Marchand, P.

AU - Masson, J.

AU - Chabrier, G.

AU - Hennebelle, P.

AU - Commercon, B.

AU - Vaytet, N.

PY - 2016/8

Y1 - 2016/8

KW - magnetohydrodynamics (MHD)

KW - ISM: molecules

KW - stars: formation

U2 - 10.1051/0004-6361/201526780

DO - 10.1051/0004-6361/201526780

M3 - Journal article

VL - 592

JO - Astronomy & Astrophysics

JF - Astronomy & Astrophysics

SN - 0004-6361

M1 - A18

ER -

ID: 174203974