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Bipolar H{\sc ii} regions produced by cloud/cloud collisions
Anthony Whitworth, Oliver Lomax, Scott Balfour +3
We suggest that Bipolar H{\sc ii} Regions may be the aftermath of collisions between clouds. Such a collision will produce a shock-compressed layer, and a star cluster can then con…
Lack of high-mass prestellar cores in the starless MDCs of NGC6334
F. Louvet, S. Neupane, G. Garay +6
Two families of models compete to explain the formation of high-mass stars. The quasi-static models predict the existence of high-mass pre-stellar cores sustained by a high degree…
ALMA observations of RCW 120 Fragmentation at 0.01pc scale
Miguel Figueira, Leonardo Bronfman, Annie Zavagno +4
Little is known about how high-mass stars form. Around 30\% of the young high-mass stars in the Galaxy are observed at the edges of ionized (HII) regions. Therefore these are place…
A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE).III. Star formation in the stripped gas of NGC 4254
A. Boselli, M. Fossati, J. C. Cuillandre +22
During pilot observations of the Virgo Environmental Survey Tracing Galaxy Evolution (VESTIGE), a blind narrow-band Halpha+[NII] imaging survey of the Virgo cluster carried out wit…