... and southern (b) Galactic polar caps versus Galactic latitude. any of the instabilities, most commonly the thermal instability that arises after initial contraction of the medium in shocks -- spiral arms or supernova remnants, is taken as an alternative ...
78. Elena Barsukova, Special Astrophysical Observatory, Russia
... N., Barbieri M., Bettoni D., Harutyunyan A., Kangas T., Kankare E., Martin J.C., Mattila S., Morales-Garoffolo A., Ochner P., Rebbapragada U.D., Terreran G., Tomasella L., Turatto M., Verroi E., Wozniak P.R. Interacting supernovae and supernova impostors ...
79. http://jet.sao.ru/jet/~bars/allpube.htm
... M., Bettoni, D., Harutyunyan, A., Kangas, T., Kankare, E., Martin, J.C., Mattila, S., Morales-Garoffolo, A., Ochner, P., Rebbapragada, U.D., Terreran, G., Tomasella, L., Turatto, M., Verroi, E., Wozniak, P.R. Interacting supernovae and supernova impostors ...
80. http://jet.sao.ru/hq/skai/article/0802.3982v1.pdf
... The FIGGS data will enable us to study the ISM of most of our sample galaxies at a linear resolution of 15 - 300 pc - i.e. comparable to the scales at which energy is injected into the ISM through supernova and stellar winds. ...