High Spatial Velocity Features in the Orion Nebula,
Internal velocities in the Orion Nebula
Internal Velocities in the Orion Nebula: Large Proper-Motion Features
New Proplyds, Outflows, Shocks, and a Reflection Nebula in M43 and the Outer Parts of the Orion Nebula
Stellar Proper Motions in the Orion Nebula Cluster
The 3D Kinematics of the Orion Nebula Cluster. II. Mass-dependent Kinematics of the Inner Cluster
The Orion nebula (M42) Herbig-Haro object, HH 201, within the tip of a molecular finger
Velocity Structure in the Orion Nebula. I. Spectral Mapping in Low-Ionization Lines
X-rays from HH 210 in the Orion nebula
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
2000-03-30T02:42:14Z/2000-09-13T23:23:13Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
European Space Agency, ODell et al., 2001, 'Proper Motions and Variability of HH Objects Near the Orion Nebula', 1.0, European Space Agency, https://doi.org/10.5270/esa-cs9ryxr