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

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

Veröffentlichungen: Beitrag in BuchBeitrag in KonferenzbandPeer Reviewed

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 ngVLAwill be a key tool in understanding the nature of these events. The highspatial 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.
OriginalspracheEnglisch
TitelScience with a Next Generation Very Large Array
Seiten177
Band517
PublikationsstatusVeröffentlicht - Dez. 2018

Publikationsreihe

ReiheAstronomical Society of the Pacific Conference Series

ÖFOS 2012

  • 103003 Astronomie
  • 103004 Astrophysik

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