Related references
Note: Only part of the references are listed.OBSERVATIONAL 5-20 μm INTERSTELLAR EXTINCTION CURVES TOWARD STAR-FORMING REGIONS DERIVED FROM SPITZER IRS SPECTRA
M. McClure
ASTROPHYSICAL JOURNAL LETTERS (2009)
THE PHYSICS OF PROTOPLANETESIMAL DUST AGGLOMERATES. III. COMPACTION IN MULTIPLE COLLISIONS
Rene Weidling et al.
ASTROPHYSICAL JOURNAL (2009)
MID-INFRARED EXTINCTION MAPPING OF INFRARED DARK CLOUDS: PROBING THE INITIAL CONDITIONS FOR MASSIVE STARS AND STAR CLUSTERS
Michael J. Butler et al.
ASTROPHYSICAL JOURNAL (2009)
Shattering and coagulation of dust grains in interstellar turbulence
Hiroyuki Hirashita et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2009)
The Growth Mechanisms of Macroscopic Bodies in Protoplanetary Disks
Jürgen Blum et al.
Annual Review of Astronomy and Astrophysics (2008)
A representative particle approach to coagulation and fragmentation of dust aggregates and fluid droplets
A. Zsom et al.
ASTRONOMY & ASTROPHYSICS (2008)
Numerical determination of the material properties of porous dust cakes
D. Paszun et al.
ASTRONOMY & ASTROPHYSICS (2008)
The infrared emission spectra of compositionally inhomogeneous aggregates composed of irregularly shaped constituents
M. Min et al.
ASTRONOMY & ASTROPHYSICS (2008)
The physics of protoplanetesimal dust agglomerates. II. Low-velocity collision properties
Doreen Langkowski et al.
ASTROPHYSICAL JOURNAL (2008)
Numerical simulation of dust aggregate collisions. II. Compression and disruption of three-dimensional aggregates in head-on collisions
Koji Wada et al.
ASTROPHYSICAL JOURNAL (2008)
Current star formation in the Ophiuchus and Perseus molecular clouds: Constraints and comparisons from unbiased submillimeter and mid-infrared surveys. II
Jes K. Jorgensen et al.
ASTROPHYSICAL JOURNAL (2008)
MODELING POROUS DUST GRAINS WITH BALLISTIC AGGREGATES. I. GEOMETRY AND OPTICAL PROPERTIES
Yue Shen et al.
ASTROPHYSICAL JOURNAL (2008)
Dust emission from the Perseus molecular cloud
S. Schnee et al.
ASTROPHYSICAL JOURNAL (2008)
Numerical simulation of density evolution of dust aggregates in protoplanetary disks. I. Head-on collisions
Toru Suyama et al.
ASTROPHYSICAL JOURNAL (2008)
Monte Carlo simulation of particle interactions at high dynamic range: Advancing beyond the googol
C. W. Ormel et al.
ASTROPHYSICAL JOURNAL (2008)
Molecular evolution and star formation: From prestellar cores to protostellar cores
Yuri Aikawa et al.
ASTROPHYSICAL JOURNAL (2008)
Coagulation, fragmentation and radial motion of solid particles in protoplanetary disks
F. Brauer et al.
ASTRONOMY & ASTROPHYSICS (2008)
A combined Spitzer and Chandra survey of young stellar objects in the serpens cloud core
E. Winston et al.
ASTROPHYSICAL JOURNAL (2007)
The relationship between the optical depth of the 9.7 μm silicate absorption feature and infrared differential extinction in dense clouds
J. E. Chiar et al.
ASTROPHYSICAL JOURNAL (2007)
Closed-form expressions for particle relative velocities induced by turbulence (Research Note)
C. W. Ormel et al.
ASTRONOMY & ASTROPHYSICS (2007)
The depletion of NO in pre-protostellar cores
M. Akyilmaz et al.
ASTRONOMY & ASTROPHYSICS (2007)
The mass function of dense molecular cores and the origin of the IMF
J. Alves et al.
ASTRONOMY & ASTROPHYSICS (2007)
Dust coagulation in protoplanetary disks: porosity matters
C. W. Ormel et al.
ASTRONOMY & ASTROPHYSICS (2007)
Large-area mapping at 850 μm.: V.: Analysis of the clump distribution in the Orion A south molecular cloud
Doug Johnstone et al.
ASTROPHYSICAL JOURNAL (2006)
The physics of protoplanetesimal dust agglomerates.: I.: Mechanical properties and relations to primitive bodies in the solar system
Juergen Blum et al.
ASTROPHYSICAL JOURNAL (2006)
The abundances of nitrogen-containing molecules during pre-protostellar collapse
D. R. Flower et al.
ASTRONOMY & ASTROPHYSICS (2006)
The influence of grain rotation on the structure of dust aggregates
D Paszun et al.
ICARUS (2006)
Quiescent and coherent cores from gravoturbulent fragmentation
RS Klessen et al.
ASTROPHYSICAL JOURNAL (2005)
Structure and mechanical properties of high-porosity macroscopic agglomerates formed by random ballistic deposition -: art. no. 115503
J Blum et al.
PHYSICAL REVIEW LETTERS (2004)
Dust dynamics in compressible magnetohydrodynamic turbulence
HR Yan et al.
ASTROPHYSICAL JOURNAL (2004)
Ambipolar-diffusion timescale, star formation timescale, and the ages of molecular clouds: Is there a discrepancy?
K Tassis et al.
ASTROPHYSICAL JOURNAL (2004)
Control of star formation by supersonic turbulence
MM Mac Low et al.
REVIEWS OF MODERN PHYSICS (2004)
Evolution of dust properties in an interstellar filament
B Stepnik et al.
ASTRONOMY & ASTROPHYSICS (2003)
Magnetic aggregation:: Dynamics and numerical Modeling
C Dominik et al.
ICARUS (2002)
Rapid formation of molecular clouds and stars in the solar neighborhood
L Hartmann et al.
ASTROPHYSICAL JOURNAL (2001)
Aluminum-26 in calcium-aluminum-rich inclusions and chondrules from unequilibrated ordinary chondrites
GR Huss et al.
METEORITICS & PLANETARY SCIENCE (2001)
Dust grain-size distributions and extinction in the Milky Way, large magellanic cloud, and small magellanic cloud
JC Weingartner et al.
ASTROPHYSICAL JOURNAL (2001)
Fractal-like aggregates: Relation between morphology and physical properties
AV Filippov et al.
JOURNAL OF COLLOID AND INTERFACE SCIENCE (2000)
Experiments on sticking, restructuring, and fragmentation of preplanetary dust aggregates
J Blum et al.
ICARUS (2000)
Share Paper
