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Star types / Nebulae / Star formation / H II region / Molecular cloud / Protostar / Stellar kinematics / Initial mass function / Star / Astronomy / Stellar astronomy / Space


Star formation in unbound giant molecular clouds: the origin of OB associations?
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City

Exeter / San Francisco / L. A. / Scoville / UNAM / Potsdam / /

Company

O N O F S TA R S A / Hillenbrand / The star / C L U S T E R S A / /

Country

Germany / Israel / Mexico / /

/

Event

Man-Made Disaster / /

Facility

University of Exeter / University of St Andrews / United Kingdom Astrophysical Fluids Facility / /

IndustryTerm

gas reservoir / gas particles / internal turbulent energy / unsupported gas / low density hydrogen gas / kinetic energy / gas surrounding / non-thermal kinetic energy / energy decay / gas expulsion / potential energy / gas stream / turbulent kinetic energy / gas expulsion phase / power-law form / unbound giant / low-density gas / gas structure / gas density / gas particle component / kinetic energy dissipation rate / gas dynamics / turbulent energy / molecular gas / positive energy / thermal energy component / /

NaturalFeature

Dale et al. / /

Organization

North Atlantic Treaty Organization / SFC / School of Physics and Astronomy / OB association / University of St Andrews / International Monetary Fund / School of Physics / Orion OB association / Cambridge Univ. / National Aeronautics and Space Administration / University of Exeter / ESA Publications Division / /

Person

Ralf Klessen / Heyer / Paul C. Clark / /

Position

author / Walker / representative / Carpenter / /

Product

Lagrangian / SFCs / /

ProvinceOrState

Texas / GMCs / Colorado / /

PublishedMedium

the Orion / /

Technology

ESA / simulation / /

URL

http /

SocialTag