ALMA observations of anisotropic dust mass loss in the inner circumstellar environment of the red supergiant VY Canis Majoris
ALMA-resolved salt emission traces the chemical footprint and inner wind morphology of VY Canis Majoris
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
Crossing the Yellow Void: Spatially Resolved Spectroscopy of the Post-Red Supergiant IRC +10420 and Its Circumstellar Ejecta
Episodic Gaseous Outflows and Mass Loss from Red Supergiants
High-Resolution, Long-Slit Spectroscopy of VY Canis Majoris: The Evidence for Localized High Mass Loss Events
Red Supergiants as Potential Type IIn Supernova Progenitors: Spatially Resolved 4.6 mm CO Emission Around VY CMa and Betelgeuse
Spatially extended K Il7699 emission in the nebula of VY CMa: kinematics and geometry
The Asymmetric Nebula Surrounding the Extreme 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
Thermal Emission in the Southwest Clump of VY CMa
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
STIS, STIS/CCD, WFPC2, WFPC2/PC
Temporal Coverage
1999-03-22T01:30:13Z/1999-09-10T12:29:50Z
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 comma Roberta M., 2000, 'High Resolution Imaging and Spectroscopy of Cool Hypergiants Near the Top of the HR Diagram', 1.0, European Space Agency, https://doi.org/10.5270/esa-1mg9w5w