Massive Star Birth Sites and the Case of NGC 3576 IRS 1

Details Massive Star Birth Sites and the Case of NGC 3576 IRS 1 Massive Star Birth Sites and the Case of NGC 3576 IRS 1

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..322..387b&link_type=abstract

The Formation and Evolution of Massive Young Star Clusters, ASP Conference Series, Vol. 322. Edited by H.J.G.L.M. Lamers, L.J.

Astronomy and Astrophysics

Astronomy

Scientific paper

We present a model for the geometry of massive star birth sites based on near and mid infrared data of NGC 3576 IRS 1. We suggest that massive stars may form via an accretion disk that eventually becomes a flared torus when the accretion ends. The differences observed among the objects and their spectral energy distribution can be explained by viewing the torus from different lines of site.

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