Disks, Microjets, Windblown Bubbles, and Outflows in the Orion Nebula

By J. Bally, C. O’Dell, M. McCaughrean. 2000

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In Astronomy and Astrophysics

Citations in the corpus

TIME EVOLUTION OF VISCOUS CIRCUMSTELLAR DISKS DUE TO PHOTOEVAPORATION BY FAR-ULTRAVIOLET, EXTREME-ULTRAVIOLET, AND X-RAY RADIATION FROM THE CENTRAL STAR (2009, result): “Subsequent observations of disks around low mass stars near the bright Trapezium O star Θ1C have confirmed the occurence of the process (e.g., Bally et al. 2000, Goto et al. 2006, Cieza et al. 2008) and observed mass loss rates correspond very well to the theoretically predicted rates (Rigliaco et…”
The Orion Nebula and Its Associated Population (2001, background): “…optical flows that appear to originate from close to Orion-S (labeled OMC1-S in Figure 11), including HH 529, HH 269, and HH 530; however, the symmetry axes of HH 529 and HH 269 clearly lie to the north of the core of Orion-S which produces the bipolar molecular outflows (Bally et al. 2000).”
HERBIG-HARO FLOWS: Probes of Early Stellar Evolution (2001, background): “Bally et al. (2000) found 21 irradiated microjets propagating into the photoionized interior of the Orion Nebula.”
The Birth of High-Mass Stars: Accretion and/or Mergers? (2005, background): “The intense UV radiation field of the Trapezium stars is photo-evaporating these disks, making them visible as Orion’s ‘proplyds’ (O’Dell, Wen, & Hu 1993; O’Dell & Wong 1996; Bally et al. 1998, 2000; Johnstone, Hollenbach, & Bally 1998; McCaughrean, Stapelfeldt, & Close 2000).”
Infrared Spectroscopy of Substellar Objects in Orion (2001, background): “047-436 lies , 1 arcmin north of the complex of bow shocks associated with LL Ori., observed in Ha by Bally et al. (2000).”