The masing environment of star forming object IRAS00338+6312: Disk, outflow, or both ?

Details The masing environment of star forming object IRAS00338+6312: Disk, outflow, or both ? The masing environment of star forming object IRAS00338+6312: Disk, outflow, or both ?

Jun 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996a%26a...310..199f&link_type=abstract

Astronomy and Astrophysics, v.310, p.199-210

Astronomy and Astrophysics

Astrophysics

34

Accretion Disks, Masers, Stars: Pre-Main Sequence, Ism: Jets And Outflows, Radio Lines: Ism, Stars: Individual: Iras 00338+6312

Scientific paper

We present results of a multi-epoch 0.1" angular resolution study of the 22GHz H_2_O maser emission towards the young stellar outflow source IRAS00338+6312. The overall maser emission consists of about a dozen individual spectral features that form a systematic position-velocity structure indicative of a pattern expected from a protostellar disk. Since it is a priori not clear whether the H_2_O maser emission originates in a disk or the associated outflow, we consider both possibilities.

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