Related references
Note: Only part of the references are listed.ON THE INITIAL CONDITIONS FOR STAR FORMATION AND THE INITIAL MASS FUNCTION
Bruce G. Elmegreen
ASTROPHYSICAL JOURNAL (2011)
The puzzle of the cluster-forming core mass-radius relation and why it matters
Genevieve Parmentier et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2011)
From the molecular-cloud- to the embedded-cluster-mass function with a density threshold for star formation
Genevieve Parmentier
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2011)
A gallery of bubbles The nature of the bubbles observed by Spitzer and what ATLASGAL tells us about the surrounding neutral material
L. Deharveng et al.
ASTRONOMY & ASTROPHYSICS (2010)
NEW TESTS FOR DISRUPTION MECHANISMS OF STAR CLUSTERS: THE LARGE AND SMALL MAGELLANIC CLOUDS
Rupali Chandar et al.
ASTROPHYSICAL JOURNAL (2010)
THE MASS-SIZE RELATION FROM CLOUDS TO CORES. II. SOLAR NEIGHBORHOOD CLOUDS
J. Kauffmann et al.
ASTROPHYSICAL JOURNAL (2010)
THE MASS-SIZE RELATION FROM CLOUDS TO CORES. I. A NEW PROBE OF STRUCTURE IN MOLECULAR CLOUDS
J. Kauffmann et al.
ASTROPHYSICAL JOURNAL (2010)
ON THE STAR FORMATION RATES IN MOLECULAR CLOUDS
Charles J. Lada et al.
ASTROPHYSICAL JOURNAL (2010)
HOW MANY INFRARED DARK CLOUDS CAN FORM MASSIVE STARS AND CLUSTERS?
Jens Kauffmann et al.
ASTROPHYSICAL JOURNAL LETTERS (2010)
The relation between the most-massive star and its parental star cluster mass
C. Weidner et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2010)
The fragmentation of expanding shells - I. Limitations of the thin-shell approximation
James E. Dale et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2009)
Search for OB stars running away from young star clusters I. NGC 6611
V. V. Gvaramadze et al.
ASTRONOMY & ASTROPHYSICS (2008)
On the origin of field O-type stars
E. Schilbach et al.
ASTRONOMY & ASTROPHYSICS (2008)
Structural analysis of molecular clouds: Dendrograms
E. W. Rosolowsky et al.
ASTROPHYSICAL JOURNAL (2008)
On the rapid collapse and evolution of molecular clouds
Bruce G. Elmegreen
ASTROPHYSICAL JOURNAL (2007)
Do O-stars form in isolation?
Richard J. Parker et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2007)
The origin of the Gaussian initial mass function of old globular cluster systems
Genevieve Parmentier et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2007)
The mass function of dense molecular cores and the origin of the IMF
J. Alves et al.
ASTRONOMY & ASTROPHYSICS (2007)
The maximum stellar mass, star-cluster formation and composite stellar populations
C Weidner et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2006)
Search for massive protostar candidates in the southern hemisphere -: II.: Dust continuum emission
MT Beltrán et al.
ASTRONOMY & ASTROPHYSICS (2006)
Connecting dense gas tracers of star formation in our galaxy to high-z star formation
JW Wu et al.
ASTROPHYSICAL JOURNAL (2005)
The origin of massive O-type field stars - II. Field O stars as runaways
WJ de Wit et al.
ASTRONOMY & ASTROPHYSICS (2005)
The star formation rate and dense molecular gas in galaxies
Y Gao et al.
ASTROPHYSICAL JOURNAL (2004)
Nucleosynthesis of heavy elements in massive stars
A Heger et al.
NUCLEAR PHYSICS A (2003)
The physical conditions for massive star formation: Dust continuum maps and modeling
KE Mueller et al.
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES (2002)
The structure of molecular clumps around high-mass young stellar objects
F Fontani et al.
ASTRONOMY & ASTROPHYSICS (2002)
Massive star formation in 100,000 years from turbulent and pressurized molecular clouds
CF McKee et al.
NATURE (2002)
High-mass protostellar candidates. II. Density structure from dust continuum and CS emission
H Beuther et al.
ASTROPHYSICAL JOURNAL (2002)
Share Paper
