Deciphering the 3D Orion Nebula. II. A Low Ionization Region of Multiple Velocity Components Southwest of th1 Ori C Confounds Interpretation of Low Velocity Resolution Studies of Temperature, Density, and Abundance
Deciphering the 3D Orion Nebula. III. Structure on the NE Boundary of the Orion-S Embedded Molecular Cloud
Deciphering the 3D Orion Nebula-IV: The HH 269 Flow Emerges from the Orion-S Embedded Molecular Cloud
Mapping the complex kinematics of LL objects in the Orion nebula
Structure and physical conditions in the Huygens region of the Orion nebula
Studies of NGC 6720 with Calibrated HST/WFC3 Emission-line Filter Images. III. Tangential Motions using AstroDrizzle Images
The impact of satellite trails on Hubble Space Telescope observations
The Nature and Frequency of Outflows from Stars in the Central Orion Nebula Cluster
Instrument
ACS, ACS/WFC, WFC3, WFC3/UVIS
Temporal Coverage
2011-12-31T10:04:02Z/2012-04-14T11:38:19Z
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, Rubin et al., 2013, 'Fine-scale Density, Temperature, and Ionization Fluctuations: Their Effect on Abundance Determinations', 1.0, European Space Agency, https://doi.org/10.5270/esa-ux4zyuw