{ "id": "astro-ph/9511095", "version": "v1", "published": "1995-11-20T17:54:57.000Z", "updated": "1995-11-20T17:54:57.000Z", "title": "Infall Collapse Solutions in the Inner Limit: Radiation Pressure and its Effects on Star Formation", "authors": [ "Jasmin Jijina", "Fred C. Adams" ], "comment": "28 pages, 7 uuencoded figs; accepted by ApJ", "journal": "Astrophys.J.462:874,1996", "doi": "10.1086/177201", "categories": [ "astro-ph" ], "abstract": "In this paper, we study infall collapse solutions for star formation in the small radius limit where the particle orbits become nearly pressure-free. We generalize previous solutions to simultaneously include the effects of both radiation pressure and angular momentum. The effects of radiation pressure can be modeled using a modified potential; for representative cases of such potentials, we obtain analytical solutions for the density and velocity fields. In general, radiation pressure limits the maximum mass of a forming star by reversing the infall when the star becomes sufficiently large. Our results imply that this maximum mass scale is given by the condition that the turnaround radius $R_R$ (the radius at which the radiation pressure force exceeds the gravitational force) exceeds the centrifugal radius $R_C$ (the angular momentum barrier). The maximum mass scale for a star forming within a rotating collapse flow with radiation pressure depends on the initial conditions, but is generally much larger than for the case of spherical infall considered previously. In particular, stars with masses $M_\\ast$ $\\sim 100$ $M_\\odot$ can form for a fairly wide range of initial conditions.", "revisions": [ { "version": "v1", "updated": "1995-11-20T17:54:57.000Z" } ], "analyses": { "keywords": [ "star formation", "inner limit", "maximum mass scale", "angular momentum", "study infall collapse solutions" ], "tags": [ "journal article" ], "note": { "typesetting": "TeX", "pages": 28, "language": "en", "license": "arXiv", "status": "editable", "inspire": 402533 } } }