A far-ultraviolet-driven photoevaporation flow observed in a protoplanetary disk
A Photoionized Herbig-Haro Object in the Orion Nebula
A spectacular jet from the bright 244-440 Orion proplyd: The MUSE NFM view
Backscattering and Line Broadening in Orion
Discovery of Crystallized Water Ice in a Silhouette Disk in the M43 Region
Disks, Microjets, Windblown Bubbles, and Outflows in the Orion Nebula
Evidence for Dust Grain Growth in Young Circumstellar Disks
Evidence for Grain Growth in the Protostellar Disks of Orion
Hubble Space Telescope WFPC2 Study of the Trapezium Cluster: The Influence of Circumstellar Disks on the Initial Mass Function
Kinematics of the Orion Trapezium Based on Diffracto-Astrometry and Historical Data
New Proplyds, Outflows, Shocks, and a Reflection Nebula in M43 and the Outer Parts of the Orion Nebula
Polycyclic Aromatic Hydrocarbon Emission in the Proplyd HST10: What is the Mechanism behind Photoevaporation?
Raman mapping of photodissociation regions
Search for Alignment of Disk Orientations in Nearby Star-forming Regions: Lupus, Taurus, Upper Scorpius, r Ophiuchi, and Orion
Silicate Emission Profiles from Low-Mass Protostellar Disks in the Orion Nebula: Evidence for Growth and Thermal Processing of Grains
The Curious Morphology and Orientation of Orion Proplyd HST-10
Instrument
STIS/NUV-MAMA, WFPC2, WFPC2/PC
Temporal Coverage
1998-04-04T01:49:13Z/1999-09-20T17:55:33Z
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, Bally et al., 2006, 'Probing Proto-Planetary Disks in the Orion Nebula', 1.0, European Space Agency, https://doi.org/10.5270/esa-q7spvb4
