|Title:||Circumstellar environments around the youngest protostars: interferometric observations and modeling
|Director of Research:||Looney, Leslie W.
|Doctoral Committee Chair(s):||Looney, Leslie W.
|Doctoral Committee Member(s):||Kemball, Athol J.; Gammie, Charles F.; Mouschovias, T. Ch.
|Department / Program:||Astronomy
|Degree Granting Institution:||University of Illinois at Urbana-Champaign
|Abstract:||This thesis presents observations and modeling
of nearby embedded sources in the earliest stage of protostellar evolution,
i.e., Class 0 young stellar objects,
using interferometric data of the
Berkeley-Illinois-Maryland Association array and the
Combined Array for Research in Millimeter-wave Astronomy.
Protostars form through gravitational collapse inside their natal envelopes,
and these circumstellar envelopes contain valuable information
about the physical processes of star formation.
In this thesis, both molecular lines and dust continuum are utilized to
investigate the nature of the collapsing envelopes.
In particular, I focus on the isolated edge-on low-mass protostar L1157.
While a large-scale (~20,000 AU) flattened envelope is detected in both
the N2H+ line and the 8 micron extinction perpendicular to
the outflow orientation,
the dust continuum shows spherical structures at scales between
~10^2 and ~10^3 AU.
The N2H+ observations not only reveal
the outer envelope that is too dim to be detected in dust continuum,
but they also unveil the kinematic structures of the flattened envelope.
The dust continuum is compared with theoretical collapse models
using radiative transfer calculation and Bayesian inference.
The modeling techniques, as well as the associated uncertainties,
The results show that a power-law envelope model with a density index p ~ 2
provides a better fit to the observations than
the simple Shu model or
the commonly-used Terebey-Shu-Cassen model.
Furthermore, I discuss the implications of the modeling results on the dust grain properties
and the constraints they place on the youngest circumstellar disk embedded inside the envelope.
|Rights Information:||Copyright 2011 Hsin-Fang Chiang
|Date Available in IDEALS:||2014-02-01