The collect and collapse process

More documents

Recommendations

Info

Sh 212 13 CO observations IRAM Deharveng et al. in preparation Ionized gas -40 km/s to -44 km/s -36.6 km/s to -38.4 km/s Filament -35.9 km/s to -36.8 km/s -32.7 km/s to -34.0 km/s -35.1 km/s to -36.1 km/s
Sh 212 Condensation 1 13CO JHK CFHT radio-continuum 1.3 cm VLA 200 Mʘ near-IR excess UC HII region dynamical age ~15000 yr B1 exciting star or earlier SED fitting tool Robitaille et al. 2007 central source ~14 Mʘ 30000 K ~18000 Lʘ envelope+disk view edge on
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 and 18: - Star formation far from the ioniz
Page 19 and 20: Does the collect and collapse proce
Page 21: Sh 212 MSX 8.3 μm MSX point-source
Page 25 and 26: The masses of the second-generation
Page 27 and 28: Massive-star formation by collect &

The collect and collapse process

Create successful ePaper yourself

Delete template?

Save as template?