Resolving the Radio Complexity of EXor and FUor-type Systems with the ngVLA - Archive ouverte HAL Access content directly
Conference Papers Year : 2018

Resolving the Radio Complexity of EXor and FUor-type Systems with the ngVLA

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1
J. A. White
  • Function : Author
M. Audard
  • Function : Author
P. Ábrahám
L. Cieza
  • Function : Author
F. C. de Miera
  • Function : Author
M. M. Dunham
  • Function : Author
J. D. Green
  • Function : Author
M. Güdel
  • Function : Author
A. Hales
  • Function : Author
L. Hartmann
  • Function : Author
K. Kadam
  • Function : Author
J. H. Kastner
  • Function : Author
Á. Kóspál
S. Perez
A. Postel
  • Function : Author
D. Ruiz-Rodriguez
  • Function : Author
C. Rab
  • Function : Author
E. I. Vorobyov
  • Function : Author
Z. Zhu
  • Function : Author

Abstract

Episodic accretion may be a common occurrence in the evolution of young pre-main sequence stars and has important implications for our understanding of star and planet formation. Many fundamental aspects of what drives the accretion physics, however, are still unknown. The ngVLA will be a key tool in understanding the nature of these events. The high spatial resolution, broad spectral coverage, and unprecedented sensitivity will allow for detailed analysis of outburst systems. The proposed frequency range of the ngVLA allows for observations of the gas, dust, and non-thermal emission from the star and disk.
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Dates and versions

insu-03666238 , version 1 (12-05-2022)

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J. A. White, M. Audard, P. Ábrahám, L. Cieza, F. C. de Miera, et al.. Resolving the Radio Complexity of EXor and FUor-type Systems with the ngVLA. Science with a Next Generation Very Large Array, ASP Conference Series, 0000, à renseigner, Unknown Region. pp.177. ⟨insu-03666238⟩
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