A likely inverse-Compton emission from the Type IIb SN 2013df
A morphological comparison between the central region in AGN and normal galaxies using HST data
A Turbulent Origin for Flocculent Spiral Structure in Galaxies
A Turbulent Origin for Flocculent Spiral Structure in Galaxies. II. Observations and Models of M33
How much hydrogen is in Type Ib and IIb supernova progenitors?
The Opacity of Spiral Galaxy Disks. IV. Radial Extinction Profiles from Counts of Distant Galaxies Seen through Foreground Disks
The opacity of spiral galaxy disks. V. Dust opacity, HI distributions and sub-mm emission
The opacity of spiral galaxy disks. VI. Extinction, stellar light and color
The Opacity of Spiral Galaxy Disks. VIII. Structure of the Cold ISM
The opacity of spiral galaxy disks. VII. The accuracy of galaxy counts as an extinction probe
The stellar mass to light ratio in the isolated spiral NGC 4414
The Type IIb Supernova 2013df and its Cool Supergiant Progenitor
The very young resolved stellar populations around stripped-envelope supernovae
Type IIb Supernova 2013df Entering into an Interaction Phase: A Link between the Progenitor and the Mass Loss
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1999-04-29T05:48:13Z/1999-04-29T12:02:53Z
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, Noll comma Keith S., 1999, 'Hubble Heritage observations of NGC 4414', 1.0, European Space Agency, https://doi.org/10.5270/esa-hgg9h4b