science
plus
.abes.fr
|
explorer
À propos de :
Mac Low M.-M.
Goto
Sponge
NotDistinct
Permalink
An Entity of Type :
foaf:Person
, within Data Space :
scienceplus.abes.fr
associated with source
document(s)
Type:
Person
New Facet based on Instances of this Class
Attributs
Valeurs
type
Person
name
Mac Low M.-M.
Mac Low Mordecai-Mark
Mac Low, Mordecai-Mark
Mac Low, M.-M.
personal mailbox
mordecai@amnh.org
familyName
Mac Low
Given name
M.-M.
Mordecai-Mark
is
relates
of
http://hub.abes.fr/edp/periodical/aa/2009/volume_504/issue_3/aa11797-09/authorship/3
http://hub.abes.fr/oup/periodical/mnras/2009/volume_398/issue_3/101111j13652966200915206x/authorship/3
http://hub.abes.fr/oup/periodical/mnras/2010/volume_404/issue_1/101111j13652966200915718x/authorship/3
http://hub.abes.fr/edp/periodical/aa/2010/volume_512/issue_2010/aa12437-09/authorship/5
http://hub.abes.fr/edp/periodical/aa/2009/volume_508/issue_1/aa11170-08/authorship/13
http://hub.abes.fr/oup/periodical/mnras/2006/volume_368/issue_2/101111j13652966200610172x/authorship/3
http://hub.abes.fr/edp/periodical/eas/2011/volume_52/issue_2011/eas1152023/authorship/6
http://hub.abes.fr/oup/periodical/mnras/2002/volume_337/issue_2/101046j13658711200205927x/authorship/3
http://hub.abes.fr/edp/periodical/aa/2021/volume_649/issue_2021/aa40077-20/authorship/4
http://hub.abes.fr/edp/periodical/aa/2018/volume_610/issue_2018/aa31836-17/authorship/5
http://hub.abes.fr/edp/periodical/aa/2018/volume_611/issue_2018/aa31698-17/authorship/3
http://hub.abes.fr/edp/periodical/aa/2019/volume_630/issue_2019/aa33970-18/authorship/3
is
Author
of
Algorithmic comparisons of decaying, isothermal, supersonic turbulence
Turbulent driving scales in molecular clouds
Modelling CO formation in the turbulent interstellar medium
Understanding the physics of the X-factor
Type Ia supernova-driven Galactic bulge wind
Hydrodynamical simulations of the decay of high-speed molecular turbulence - II. Divergence from isothermality
Hydrodynamical simulations of the decay of high-speed molecular turbulence — I. Dense molecular regions
Comparing the statistics of interstellar turbulence in simulations and observations
Fast methods for tracking grain coagulation and ionization
On the fragmentation of filaments in a molecular cloud simulation
Spectral shifting strongly constrains molecular cloud disruption by radiation pressure on dust
How do velocity structure functions trace gas dynamics in simulated molecular clouds?
Alternative Linked Data Documents:
ODE
Content Formats:
RDF
ODATA
Microdata
