ALMA Reveals Hidden Morphologies in the Molecular Envelope of VY Canis Majoris
An Interferometric Spectral Line and Imaging Survey of VY Canis Majoris in the 345 GHz Band
Massive dust clumps in the envelope of the red supergiant VY Canis Majoris
The Circumstellar Environments of the Cool Hypergiants: Implications for the Mass Loss Mechanism
The Mass-loss History of the Red Hypergiant VY CMa
The Three-Dimensional Morphology of VY Canis Majoris. II. Polarimetry and the Line-of-Sight Distribution of the Ejecta
The Three-Dimensional Morphology of VY Canis Majoris. I. The Kinematics of the Ejecta
The Unexpected Spectrum of the Innermost Ejecta of the Red Hypergiant VY CMa
Instrument
ACS, ACS/HRC, WFPC2, WFPC2/PC
Temporal Coverage
2004-08-17T22:39:41Z/2005-06-13T04:25:32Z
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, Humphreys et al., 2005, 'The 3D Morphology of the Extreme Red Supergiant VY CMa', 1.0, European Space Agency, https://doi.org/10.5270/esa-fml5pz4