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Temperature Fluctuations and Evolution of Dust Grains in Dense Interstellar Clouds
Published online by Cambridge University Press: 04 August 2017
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Interstellar extinction studies (Chlewicki et al, 1984), as well as IR observations (Sellgren et al, 1983) require the presence in the interstellar medium of a substantial number of small (a≲0.01 μm) dust grains. The temperature of such small grains is subjected, because of their small steady-state energy, to large fluctuations as they absorb photons from the incident radiation, which could prevent the accretion on such grains (Greenberg and Hong, 1974).
- Type
- I. Star Forming Processes in the Solar Neighborhood
- Information
- Symposium - International Astronomical Union , Volume 115: Star Forming Regions , 1987 , pp. 88 - 89
- Copyright
- Copyright © Reidel 1987
References
Aiello, S., Barsella, B., Ferrini, F., Iorio, D., Rosolia, A.: 1984, Nuovo Cimento, 7, 840
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Chlewicki, G., Greenberg, J.M., Aiello, S., Barsella, B., Patriarchi, P., Perinotto, M.: 1984, Proc 4th European IUE Conf., ESA SP-218, 507
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