Questions that Remain to be Answered...

3/15/00


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Table of Contents

Questions that Remain to be Answered...

ìClumpî Mass Distribution

A New Proposal: Episodic ejections from precessing or wobbling moving source

PV Ceph

PV Ceph 12CO (2-1) Outflow Contours on 13CO (1-0) Map

Position-Velocity Diagram for PV Ceph Outflow

PV C eph: CO (2-1) Spectra Near HH315 B

The ìBlueî Lobe of the PV Ceph Outflow

B5-IRS 5: An ìOutflowî Component?

HH300 & B18w in Taurus

The Taurus Dark Cloud Complex

4. How much of a molecular cloud complex was ìmovedî to its present location by an outflow?

YSO Outflows Move More Gas than WeThought

Author: Alyssa Goodman

Email: agoodman@cfa.harvard.edu

Home Page: cfa-www.harvard.edu/~agoodman

Other information:
Not for public use. These are primarily private comments between collaborators.

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