The W4 chimney/superbubble
Astrophysics
2007-05-23 v1
Abstract
A conical void in the Galactic HI within the Perseus arm has been proposed to be a chimney. However, Halpha data suggest that the structure may be closed at higher latitudes and therefore is a superbubble rather than a chimney. Recent observations have extended our view of the HI and the radio continuum emission to higher latitudes, up to 8 degrees;. The new images show the HI structure to be open at the top and a small filament suggests recent breakout. The conical shape of the structure is not easily explained by superbubble models.
Cite
@article{arxiv.astro-ph/0007425,
title = {The W4 chimney/superbubble},
author = {Magdalen Normandeau},
journal= {arXiv preprint arXiv:astro-ph/0007425},
year = {2007}
}
Comments
4 pages, 1 figure, to appear in the proceedings of "Stars, Gas and Dust in Galaxies: Exploring the links",eds. D. Alloin, G. Galaz, K. Olsen