Bright Hot Impacts by Erupted Fragments Falling Back on the Sun: A Template for Stellar Accretion

Author:

Reale Fabio12,Orlando Salvatore2,Testa Paola3,Peres Giovanni12,Landi Enrico4,Schrijver Carolus J.5

Affiliation:

1. Dipartimento di Fisica e Chimica, Università di Palermo, Piazza del Parlamento 1, 90134 Palermo, Italy.

2. Istituto Nazionale di Astrofisica (INAF)/Osservatorio Astronomico di Palermo, Piazza del Parlamento 1, 90134 Palermo, Italy.

3. Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, MS 58, Cambridge, MA 02138, USA.

4. Department of Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arbor, MI 48109, USA.

5. Lockheed Martin Advanced Technology Center, Palo Alto, CA 94304, USA.

Abstract

Accretion Analog Mass flow from a circumstellar disk onto a young star's surface plays an important role in the final stages of star formation but the details of this complex process are not well understood. Reale et al. (p. 251 , published online 20 June) analyzed a solar flare that led to bright impacts of plasma onto the solar surface. Numerical simulations suggest that these events can be seen as analogs to accretion of matter onto stars and can thus be used to understand stellar accretion.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference40 articles.

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