The collect and collapse process

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The collect and collapse process

The collect and collapse process

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APEX Laboca<br />

870 μm<br />

Science Verification<br />

July 2007

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EAA_ws1314_V14_summary.pdf

Vorlesung

6.1. Spektrallinien

Künstlicher Stern über dem Calar Alto (Teil 2)

Near-infrared luminosity function of galaxies in distant clusters

Max-Planck-Institut für Astronomie - Jahresbericht 2007

Max-Planck-Institut für Astronomie - Jahresbericht 2009

Annual Report 2010

thesis pdf, 3MB

L4 Star formation Part III

Where lies the Peak of the Brown Dwarf Binary Separation ...

Sterrewacht Leiden - FTP Directory Listing

Annual Report 2011 Max Planck Institute for Astronomy

Trapezoidal Rule Integration

Science Case

APEX Laboca 870 μm Science Verification July 2007

Does the <strong>collect</strong> <strong>and</strong> <strong>collapse</strong> <strong>process</strong> work in an inhomogeneous medium?

Page 1 and 2: Massive-star formation triggered by
Page 3 and 4: Different processes triggering star
Page 5 and 6: Signatures of RDI: example BRC37 Pr
Page 7 and 8: Signatures of C&C: for example RCW
Page 9 and 10: Dense molecular condensations, pote
Page 11 and 12: RCW120 Zavagno et al. 2007, A&A in
Page 13 and 14: Star formation in RCW 120 with Spit
Page 15 and 16: Spitzer-MIPS 24 μm IRAC colors and
Page 17: - Star formation far from the ioniz
Page 21 and 22: Sh 212 MSX 8.3 μm MSX point-source
Page 23 and 24: Sh 212 Condensation 1 13CO JHK CFHT
Page 25 and 26: The masses of the second-generation
Page 27 and 28: Massive-star formation by collect &