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2000ApJ...542..925L - Astrophys. J., 542, 925-945 (2000/October-3)
CO outflows from young stars: confronting the jet and wind models.
LEE C.-F., MUNDY L.G., REIPURTH B., OSTRIKER E.C. and STONE J.M.
Abstract (from CDS):
Thus, these observations provide examples of systems that support either the wide-angle wind-driven or jet-driven model in the simplest interpretation. More detailed calculations are needed to understand whether one model might be able to fit all systems. It is crucial to know if time-dependent or long-lived jet-driven bow shock models can produce the observed outflow widths and parabolic PV structures, or if a wide-angle wind can produce the shock features and velocity spur structures in our observations.
Abstract Copyright: ∼
Journal keyword(s): ISM: Individual: Alphanumeric: VLA 05487 - ISM: Individual: Alphanumeric: HH 212 - ISM: Individual: Alphanumeric: HH 240/241 - ISM: Individual: Alphanumeric: HH 111 - ISM: Individual: Alphanumeric: RNO 91 - ISM: Jets and Outflows - Stars: Formation
Errata: Erratum vol. 549, p. 1231 (2001)
CDS comments: VLA 05487 = [DME94] HH 110 IRS 2
Simbad objects: 33
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