A Dust-Scattering Model for M1-92: A Revised Estimate of the Mass Distribution and Inclination
Fast, Gusty Winds Blowing from the Core of the Pre-planetary Nebula M 2-56
Hubble Space Telescope and Ground-based Imaging of the Bipolar Proto--Planetary Nebula M1-92: Evidence for a Collimated Outflow
IRAS 17423-1755 (Hen 3-1475) Revisited: An O-rich High-mass Post-asymptotic Giant Branch Star
Multiple Collimated Outflows in the Proto-Planetary Nebula GL 618
Multiple Molecular H2 Outflows in AFGL 618
Near-infrared spectroscopy of (proto)-planetary nebulae: molecular hydrogen excitation as an evolutionary tracer
New light on the multiple jets of CRL 618
Outflows from Evolved Stars: The Rapidly Changing Fingers of CRL 618
Physical Structure of the Protoplanetary Nebula CRL 618. II. Interferometric Mapping of Millimeter-Wavelength HCN J = 1-0, HCO+ J = 1-0, and Continuum Emission
Physical Structure of the Proto-Planetary Nebula CRL 618. I. Optical Long-Slit Spectroscopy and Imaging
Shaping Proto-Planetary and Young Planetary Nebulae with Collimated Fast Winds
STIS optical spectroscopy of the lobes of CRL 618
The Emerging Planetary Nebula CRL 618 and its Unsettled Central Star(s)
Watching PrePNe Evolve: 15 Years of HST Observations
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1996-04-24T21:47:16Z/1998-10-23T17:33:14Z
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, Trammell et al., 1999, 'The Origin of Shock Emission in Proto- Planetary Nebulae', 1.0, European Space Agency, https://doi.org/10.5270/esa-z87n4eu
