Rohde, P. F., Walch, S., Seifried, D., Whitworth, A. P. and Clarke, S. D. (2022). Protostellar outflows: a window to the past. Mon. Not. Roy. Astron. Soc., 510 (2). S. 2552 - 2572. OXFORD: OXFORD UNIV PRESS. ISSN 1365-2966

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Abstract

During the early phases of low-mass star formation, episodic accretion causes the ejection of high-velocity outflow bullets, which carry a fossil record of the driving protostar's accretion history. We present 44 SPH simulations of 1 M-circle dot cores, covering a wide range of initial conditions, and follow the cores for five free-fall times. Individual protostars are represented by sink particles, and the sink particles launch episodic outflows using a sub-grid model. The OPTICS algorithm is used to identify individual episodic bullets within the outflows. The parameters of the overall outflow and the individual bullets are then used to estimate the age and energetics of the outflow, and the accretion events that triggered it, and to evaluate how reliable these estimates are, if observational uncertainties and selection effects (like inclination) are neglected. Of the commonly used methods for estimating outflow ages, it appears that those based on the length and speed of advance of the lobe are the most reliable in the early phases of evolution, and those based on the width of the outflow cavity and the speed of advance are most reliable during the later phases. We describe a new method that is almost as accurate as these methods, and reliable throughout the evolution. In addition, we show how the accretion history of the protostar can be accurately reconstructed from the dynamics of the bullets if each lobe contains at least two bullets. The outflows entrain about 10 times more mass than originally ejected by the protostar.

Item Type: Journal Article
Creators:
CreatorsEmailORCIDORCID Put Code
Rohde, P. F.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Walch, S.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Seifried, D.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Whitworth, A. P.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Clarke, S. D.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
URN: urn:nbn:de:hbz:38-666547
DOI: 10.1093/mnras/stab3572
Journal or Publication Title: Mon. Not. Roy. Astron. Soc.
Volume: 510
Number: 2
Page Range: S. 2552 - 2572
Date: 2022
Publisher: OXFORD UNIV PRESS
Place of Publication: OXFORD
ISSN: 1365-2966
Language: English
Faculty: Unspecified
Divisions: Unspecified
Subjects: no entry
Uncontrolled Keywords:
KeywordsLanguage
YOUNG STELLAR OBJECTS; MAGNETOCENTRIFUGALLY DRIVEN FLOWS; PROBING EPISODIC ACCRETION; HERBIG-HARO FLOWS; STAR-FORMATION; MOLECULAR OUTFLOWS; HIGH-VELOCITY; RADIATIVE FEEDBACK; ALMA OBSERVATIONS; BIPOLAR OUTFLOWMultiple languages
Astronomy & AstrophysicsMultiple languages
URI: http://kups.ub.uni-koeln.de/id/eprint/66654

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