SIMBAD references

2014MNRAS.444.3657P - Mon. Not. R. Astron. Soc., 444, 3657-3669 (2014/November-2)

Kompaneets model fitting of the Orion-Eridanus superbubble.

PON A., JOHNSTONE D., BALLY J. and HEILES C.

Abstract (from CDS):

Winds and supernovae from OB associations create large cavities in the interstellar medium referred to as superbubbles. The Orion molecular clouds are the nearest high-mass star-forming region and have created a highly elongated, 20°x45°, superbubble. We fit Kompaneets models to the Orion-Eridanus superbubble and find that a model where the Eridanus side of the superbubble is oriented away from the Sun provides a marginal fit. Because this model requires an unusually small scaleheight of 40 pc and has the superbubble inclined 35° from the normal to the Galactic plane, we propose that this model should be treated as a general framework for modelling the Orion-Eridanus superbubble, with a secondary physical mechanism not included in the Kompaneets model required to fully account for the orientation and elongation of the superbubble.

Abstract Copyright: © 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2014)

Journal keyword(s): stars: formation - ISM: bubbles - ISM: clouds - ISM: individual objects: Orion - ISM: structure

Status in Simbad:  being processed

Simbad objects: 23

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2019.12.07-12:32:53

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