HERBIG-HARO FLOWS: Probes of Early Stellar Evolution

By B. Reipurth, J. Bally. 2001

511 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics

View Paper: https://www.semanticscholar.org/paper/e771da1409f3ed02ea5a27bff9ccdc18810e7ce2

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Citations in the corpus

LOCAL STUDY OF ACCRETION DISKS WITH A STRONG VERTICAL MAGNETIC FIELD: MAGNETOROTATIONAL INSTABILITY AND DISK OUTFLOW (2012, background): “In particular, the presence of jets and outflows in a wide range of accretion systems such as protostars (e.g., Reipurth & Bally 2001; Cabrit 2007), X-ray binaries (e.g., Mirabel & Rodŕıguez 1999; Fender 2006) and active galactic nuclei (e.g., Begelman et al. 1984; Harris & Krawczynski 2006) is…”
Magnetic tower outflows from a radial wire array Z-pinch (2005, background): “On more easily observable scales, the collimated outflows appear to be super-Alfvenic (Reipurth and Bally 2001).”
THE INTERPLAY OF MAGNETIC FIELDS, FRAGMENTATION, AND IONIZATION FEEDBACK IN HIGH-MASS STAR FORMATION (2010, background): “This structure is a magnetic bubble rather than the outflow we are familiar with in low-mass star formation (Cabrit & André 1991; Bachiller 1996; Reipurth & Bally 2001; Bally et al. 2007).”
Accretion-powered Stellar Winds. II. Numerical Solutions for Stellar Wind Torques (2008, background): “The pre-main-sequence phase is, in fact, marked by powerful outflows (Reipurth & Bally 2001).”
The Birth of High-Mass Stars: Accretion and/or Mergers? (2005, background): “Disk accretion in forming low-mass stars produces highly collimated jets (e.g. Reipurth & Bally 2001).”
The Far-Ultraviolet Spectrum of TW Hydrae. I. Observations of H2 Fluorescence (2002, background): “The extended IR H2 emission seen around T Tau and other young embedded sources such as L1448 (Bally, Lada, & Lane 1993) is interpreted as shock-heated emission from the interaction of the stellar/disk wind/jet with the surrounding cloud material (see review by Reipurth & Bally 2001).”
A COLD COMPLEX CHEMISTRY TOWARD THE LOW-MASS PROTOSTAR B1-b: EVIDENCE FOR COMPLEX MOLECULE PRODUCTION IN ICES (2010, background): “If an outflow is still active in the direction of the ‘core’ position, the UV radiation may originate in the jet shock itself (Reipurth & Bally 2001).”
Star formation through gravitational collapse and competitive accretion (2006, background): “Energy injection from jets and outflows is relatively quick with typical dynamical times of the flows is generally of order 103 to 104 years (e.g. Reipurth & Bally 2001; Beuther et al. 2002).”
On the Evolutionary Status of Class I Stars and Herbig-Haro Energy Sources in Taurus-Auriga (2004, background): “At least 60% of all class I objects are associated with Herbig-Haro (HH) objects (Gomez et al. 1997; Kenyon et al. 1998; Reipurth 1999), which are regions of shocked gas believed to be powered by an outflow or jet (Reipurth & Bally 2001).”
Probing T Tauri Accretion and Outflow with 1 Micron Spectroscopy (2006, background): “Knowledge of accretion driven winds comes primarily from spatially extended collimated atomic and molecular jets comprised of high velocity (200−400 km s−1) outflowing material undergoing internal shocks (Hartigan et al. 1995; Reipurth & Bally 2001; Hartigan et al. 2004).”