Astron. J., 125, 277-287 (2003/January-0)
High proper motion features in the central Orion nebula.
O'DELL C.R. and DOI T.
Abstract (from CDS):
The brightest portion of the Orion Nebula has been reimaged with the Hubble Space Telescope in Hα, [N II], and [O III]. Comparison with earlier Wide Field Planetary Camera 2 images going back as much as 8 yr has allowed determination of tangential velocities (proper motions) down to about 10 km.s–1 for a variety of sources. Multiple outflow systems are found associated with individual proplyds in the ionized portion of the nebula (HH 518, HH 624, possibly HH 507). The Orion-S complex of radio and infrared sources is the source of multiple outflows. A new outflow system (HH 625) has been identified as coming from the blueshifted portion of the imbedded high velocity CO flow coming from the Orion-S region, this object having CO, H2, and low ionization optical components. The low velocity CO outflow originating from or near FIR 4 is the likely source of HH 530. A new imbedded source is inferred from this optical data to lie in Orion-S. This optical outflow source (OOS) clearly feeds the systems HH 269 and HH 529, which lie along a straight line. There is evidence that this is also the source for HH 528, HH 202, and HH 203/204, all of which are blueshifted (except possibly HH 528 whose radial velocity is unknown). There is no strong radio, infrared, or X-ray source within the positional ellipse of the OOS.
ISM: Herbig-Haro Objects - ISM: Individual: Name: Orion Nebula - ISM: Jets and Outflows - Stars: Winds, Outflows
VizieR on-line data:
<Available at CDS (J/AJ/125/277): table1.dat>
Table 1: [OW94] SSs-MMSW N=70
erratum vol. 125, p. 2753 (2003)
FIR 4 = [MWZ90] OMC-1 FIR 4
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