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Herbig-Haro objects and post-FUOR's
Astrophysics, 1976In this work, we propose that the Herbig-Haro objects can be divided into two groups. Objects in the first group have luminosities which can be quantitatively explained by reflection of the light from a neighboring source. Objects in the second group are not illuminated from outside.
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An Extended Catalog of Herbig–Haro Objects
Research in Astronomy and AstrophysicsAbstract We present an extended catalog of 1193 Herbig–Haro (HH) objects, comprising 477 isolated HH objects and 716 HH knots, compiled through a meticulous review of the literature available through mid-2025. The catalog provides comprehensive data for each entry, including celestial coordinates, distances, knot separations, exciting
Zhi-Yu Chen, Chao-Jian Wu
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Herbig–Haro Objects and Protoplanetary Discs
2010Herbig–Haro objects are associated with T Tau stars, being the structures that were formed from their winds. Also, the discs that form in the planetary nebulae are very similar to the protoplanetary ones and the dynamics they generate is very similar, so the models used to explain them are also applicable here. Information on the characteristics of the
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New Herbig–Haro objects and outflows in the Mon R1 association
Monthly Notices of the Royal Astronomical Society, 2020S N Dodonov, T A Movsessian
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Herschelobservations of the Herbig-Haro objects HH 52-54
Astronomy and Astrophysics, 2011Odysseas Dionatos +2 more
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Herbig-Haro Flows: Probes of Early Stellar Evolution
Annual Review of Astronomy and Astrophysics, 2001John Bally, Bo Reipurth
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The outflow history of two Herbig-Haro jets in RCW 36: HH 1042 and HH 1043
Astronomy and Astrophysics, 2013Hugues Sana +2 more
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