Abstract
The Discussion has been rearranged into five sections: 1. Density Concentrations, Cocoon Stars, and OH Sources; 2. The Carbon Recombination Line; 3. The He/H Abundance; 4. Various Shorter Comments; 5. A New Mechanism for Star Formation. A part of the Discussion which related to Spiegel’s Report has been transferred to Chapter 13. A short exchange on HI shells around HII regions has been deleted and added to Chapter 5. A short part on the dust cloud in Orion at the end of Section 4 has been transferred from Tuesday, September 16.
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© 1970 IAU
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Shklovskii, I.S. (1970). Discussion Following Mezger’s Report. In: Habing, H.J. (eds) Interstellar Gas Dynamics. International Astronomical Union/Union Astronomique Internationale, vol 39. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-3329-9_26
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DOI: https://doi.org/10.1007/978-94-010-3329-9_26
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-3331-2
Online ISBN: 978-94-010-3329-9
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