A Collimated, Ionized Bipolar Structure and a High Density Torus in the Planetary Nebula IRAS 17347-3139
A Molecular-line Study of the Interstellar Bullet Engine IRAS05506+2414
A Quadrupolar Preplanetary Nebula: IRAS 19475+3119
A Starfish Preplanetary Nebula: IRAS 19024+0044
A Study of H2 Emission in Three Bipolar Proto-Planetary Nebulae: IRAS 16594-4656, Hen 3-401, and Rob 22
High-Velocity Interstellar Bullets in IRAS 05506+2414: A Very Young Protostar
Large-scale environments of binary AGB stars probed by Herschel. II. Two companions interacting with the wind of p1 Gruis
OPACOS: OVRO Post-AGB CO (1-0) Emission Survey. I. Data and Derived Nebular Parameters
Preplanetary Nebulae: A Hubble Space Telescope Imaging Survey and a New Morphological Classification System
Probing the fast outflow in IRAS 15452 - 5459 with ATCA observations of OH, H2O and SiO masers
Revealing the Mid-Infrared Emission Structure of IRAS 16594-4656 and IRAS 07027-7934
The Spatio-Kinematical Structure and Distance of the Preplanetary Nebula IRAS 19134+2131
Instrument
NICMOS, NICMOS/NIC1, NICMOS/NIC2
Temporal Coverage
2003-07-14T17:10:16Z/2004-04-25T11:18:46Z
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, Sahai comma Raghvendra, 2005, 'Are OH/IR Stars the Youngest post-AGB stars? A NICMOS Imaging Survey', 1.0, European Space Agency, https://doi.org/10.5270/esa-g7boh1w