The collect and collapse process

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RCW 79 second-generation exciting cluster JHK ESO Ionization front & associated PAHs emission second-generation HII region & associated PAHs emission UC HII region observed in the direction of the <strong>collect</strong>ed layer first-generation HII region Spitzer-Glimpse 8 μm
Dense molecular condensations, potential sites of star formation, can also be formed by Dynamical instabilities of the ionization front Garcia-Segura & Franco 1996 Mizuta et al. 2006 or by Turbulence Elmegreen, Kimura & Tosa 1995 Dale et al. 2005 Gritschneder, Heitsch & Burkert 2006
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: Signatures of C&C: for example RCW
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 and 18: - Star formation far from the ioniz
Page 19 and 20: Does the collect and collapse proce
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 &

The collect and collapse process

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