Hostname: page-component-76fb5796d-9pm4c Total loading time: 0 Render date: 2024-04-25T15:55:03.660Z Has data issue: false hasContentIssue false
  • English
  • Français

Young Stars and Planets Near the Sun: Explosive Phenomena from Falling Evaporating Bodies

Published online by Cambridge University Press:  27 January 2016

Subhon Ibadov  and
Firuz S. Ibodov
Subhon Ibadov
Affiliation:
Lomonosov Moscow State University, Sternberg Astronomical Institute, 119991 Moscow, Russia email: mshtf@sai.msu.ru Institute of Astrophysics, Tajik Academy of Sciences, 734042 Dushanbe, Tajikistan email: ibadovsu@yandex.ru
Firuz S. Ibodov
Affiliation:
Lomonosov Moscow State University, Sternberg Astronomical Institute, 119991 Moscow, Russia email: mshtf@sai.msu.ru
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Impacts of falling evaporating bodies (FEBs) with stars and planets at velocities V ≳ 10 − 20 km/s will be accompanied, due to aerodynamic effects such as crushing and transversal expansion of the crushed mass, by the FEB's “explosion” and the generation of a strong “blast” wave, resulting in FEB-generated explosive/flare phenomena. Multiwavelength monitoring of nearby young stars (and exoplanets) with dense protoplanetary disks rich in FEB's is hence of interest for identifying such FEB-related mechanisms possibly underlying their variability.

Keywords

Young starsfalling evaporating bodiesFEB-generated explosive/flare phenomena
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Issue S314: Young Stars & Planets Near the Sun , November 2015 , pp. 253 - 254
Copyright
Copyright © International Astronomical Union 2016 

References

Eichler, D. & Mordecai, D. 2012, ApJL, 761, L27Google Scholar
Grigorian, S. S., Ibadov, S., & Ibodov, F. S. 2000, D-Ph, 45, 463Google Scholar
Grigorian, S. S., Ibodov, F. S., & Ibadov, S. I. 2013, Sol. Sys. Res., 47, 268Google Scholar
Ibadov, S. 1990, Icarus, 86, 283CrossRefGoogle Scholar
Ibadov, S. 2011, in Proc.IAUS 283, Manchado, A., Stanghellini, L., & Schonberner, D., eds., p. 392Google Scholar
Ibadov, S. 2012, Adv.Space Res., 49, 467Google Scholar
Ibadov, S., Ibodov, F. S. & Grigorian, S. S. 1999, Rom. As. J Suppl, 9, 125Google Scholar
Ibadov, S.et al. 2009, in Proc. IAUS 257, Gopalswamy, N. & Webb, D. F., eds., p. 341Google Scholar
Ibodov, F. S. & Ibadov, S. 2014, in Proc. IAUS 300, Schmieder, B.et al., eds., p. 509.Google Scholar
Lagrange, A. M., Ferlet, R., & Vidal-Madjar, A. 1987, A&A, 173, 289Google Scholar
Schrijver, C. J., Brown, J. C., Battams, K., et al. 2012, Science, 335, 324Google Scholar
Teets, W. K., Weintraub, D. A., Grosso, N., et al. 2011, ApJ, 741, 83Google Scholar
Weissman, P. R. 1983, Icarus, 55, 448Google Scholar