Kinematics of Herbig-Haro Objects and Jets in the Orion Nebula

Abstract

We have surveyed the inner 5' of the Orion Nebula by means of Halpha and [NII] Fabry-Perot imaging spectroscopy to present a kinematical study of the Herbig-Haro objects in the nebula. The objects studied in this work are HH 202, 203, 204, 529, 269 and other associated features. For HH 202 we find new features that, because of their high velocities (up to 100 km/seg) indicate the presence of an outflow that probably is a HH flow not catalogued previously. HH 202 could be only a part of this larger outflow. Large internal motions are found in the fainter regions of HH 203-204, as well as evidence of transverse density gradients that could account for the asymmetry in the brightness distribution of HH 204. We report for the first time a high blueshifted velocity (-118 km/seg) associated with HH 204, and show that the apex of HH 204 is indeed the zone of maximum velocity, in agreement with bow shock models. We also studied the radial velocity field of HH 269 finding features associated with the HH object. From our studies, we find kinematic evidence that suggests that HH 203-204 and HH 202 are part of a big (aprox. 0.55 pc) bipolar HH outflow.

24 pages, 10 figures (in three jpg files). To be Published in Astronomical Journal

References in corpus (1)

• Kinematics of Herbig-Haro Objects and Jets in the Orion Nebula

Cited by in corpus (10)

• A MUSE map of the central Orion Nebula (M 42)
• The Orion Nebula in the mid-IR
• Silicon Monoxide Observations Reveal a Cluster of Hidden Compact Outflows in the OMC1 South Region
• A Cluster of 1.3 cm Continuum Sources in OMC1 South
• Velocity Structure in the Orion Nebula. I. Spectral Mapping in Low-Ionization Lines
• Large Scale Flows from Orion-South
• Thermal-IR Detection of Optical Outflow Sources in OMC1 South
• Kinematics of Herbig-Haro Objects and Jets in the Orion Nebula
• Exploring the effects of high-velocity flows in abundance determinations in H II regions. Bidimensional spectroscopy of HH 204 in the Orion Nebula
• Near-Infrared Polarization Images of The Orion Molecular Cloud 1 South Region