A Dust-Scattering Model for M1-92: A Revised Estimate of the Mass Distribution and Inclination
Near-infrared spectroscopy of (proto)-planetary nebulae: molecular hydrogen excitation as an evolutionary tracer
The shock structure in the protoplanetary nebula M1-92: imaging of atomic and H_2 line emission
Unveiling shocks in planetary nebulae
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1996-05-30T13:34:16Z/1996-05-30T19:03:56Z
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, Bujarrabal comma Valentin, 1997, 'Shocks in protoplanetary nebulae', 1.0, European Space Agency, https://doi.org/10.5270/esa-84kwt5p