CO Outflows from Young Stars: Confronting the Jet and Wind Models

By Chin-Fei Lee, L. Mundy, B. Reipurth, E. Ostriker, James M. Stone. 2000

170 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Spectroscopy

View Paper: https://www.semanticscholar.org/paper/2327fedb2432b24a81141084660c0f4aac04a845

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. E. Ostriker
2. Masahiro N. Machida
3. Zhi-Yun Li
4. Mark R. Krumholz
5. K. Tomida
6. C. McKee
7. Tomoaki Matsumoto
8. Matthew R. Bate

In Spectroscopy

1. E. Ostriker
2. Zhi-Yun Li
3. C. McKee
4. A. Sargent
5. H. Arce
6. S. Okuzumi
7. B. Reipurth
8. Christoph Federrath

Citations in the corpus

• RADIATION MAGNETOHYDRODYNAMIC SIMULATIONS OF PROTOSTELLAR COLLAPSE: PROTOSTELLAR CORE FORMATION (2012, result): “If this is the case, our simulations can naturally explain the observed high-velocity jets, especially the multi-component outflows (for example, Lee et al. 2000; Santiago-Garcı́a et al. 2009).”
• Theory of Star Formation (2007, background): “Channel maps and position-velocity diagrams in some sources show parabolic structures that are consistent with driving by wide-angle winds, and in other sources show spur structures that are consistent with jet driving (Lee et al., 2000, 2001).”
• Magnetocentrifugal Launching of Jets from Accretion Disks. II. Inner Disk-driven Winds (2003, background): “The combination of external and intrinsic collimation may produce a more jet-dominated magnetocentrifugal wind; such a wind may be needed to explain the kinematics of some bipolar molecular outflows (Lee et al. 2000).”
• A study of high velocity molecular outflows with an up-to-date sample (2004, background): “Now it is believed that low mass outflows are driven by bow shocks (Lee et al. 2000; Chernin & Masson 1995; Raga & Cabrit 1993; de Young 1986) while wide-angle wind may drive massive outflows (Molinari et al. 2002).”
• HERBIG-HARO FLOWS: Probes of Early Stellar Evolution (2001, background): “Some outflows appear to be best explained by one model, whereas others are best fit by the other (e.g., Nagar et al. 1997, Gueth & Guilloteau 1999, Lee et al. 2000).”
• The Evolution of Outflow-Envelope Interactions in Low-Mass Protostars (2006, methodology): “Based on singledish and interferometer maps at higher angular resolution, the molecular outflow has been successfully modeled as a slowly expanding shell driven by a wide-angle wind (Bence et al. 1998; Lee et al. 2000, 2001; Lee & Ho 2005).”