STAR FORMATION AND THE NATURE OF BIPOLAR OUTFLOWS

Research output: Journal Publications and Reviews (RGC: 21, 22, 62) › 21_Publication in refereed journal › peer-review

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Author(s)

Detail(s)

Original languageEnglish
Pages (from-to)L31-L34
Journal / PublicationAstrophysical Journal
Volume370
Issue number1 PART 2
Publication statusPublished - 20 Mar 1991
Externally publishedYes

Link(s)

DOI

DOI
Check@CityULib
Link to Scopus https://www.scopus.com/record/display.uri?eid=2-s2.0-4243968532&origin=recordpage
Permanent Link https://scholars.cityu.edu.hk/en/publications/publication(4f38112a-09dc-482d-aa3a-eaeacc2ade5b).html

Abstract

We present a simple physical model for the bipolar molecular outflows that frequently accompany star formation. Our model forges an intrinsic link between the bipolar flow phenomenon and the process of star formation, and it helps to explain many of the systematics known for existing sources.

Research Area(s)

  • Hydrodynamics, Nebulae: internal motions, Stars: formation, Stars: mass loss, Stars: pre-main-sequence

Citation Format(s)

[ RIS ] [ BibTeX ]

STAR FORMATION AND THE NATURE OF BIPOLAR OUTFLOWS. / SHU, Frank H.; RUDEN, Steven P.; LADA, Charles J. et al.

In: Astrophysical Journal, Vol. 370, No. 1 PART 2, 20.03.1991, p. L31-L34.

Research output: Journal Publications and Reviews (RGC: 21, 22, 62) › 21_Publication in refereed journal › peer-review