A Critical Examination of Hypernova Remnant Candidates in M101. II. NGC 5471B
A Critical Examination of Hypernova Remnant Candidates in M101. I. MF 83
Clusters in the Luminous Giant H II Regions in M101
Giant H II Regions in M101. I. X-Ray Analysis of Hot Gas
Internal kinematics of giant H II regions in M101 with the Keck Cosmic Web Imager
Millimeter Observations of the Type II SN 2023ixf: Constraints on the Proximate Circumstellar Medium
Physical Structure and Nature of Supernova Remnants in M101
SN 2023ixf in Messier 101: A Variable Red Supergiant as the Progenitor Candidate to a Type II Supernova
SN 2023ixf in Messier 101: The Twilight Years of the Progenitor as Seen by Pan-STARRS
Star formation in NGC5471
Star formation in OB associations and clusters
The 100 Myr Star Formation History of NGC 5471
The Dusty Red Supergiant Progenitor and the Local Environment of the Type II SN 2023ixf in M101
The Vast Population of Wolf-Rayet and Red Supergiant Stars in M101. I. Motivation and First Results
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1997-11-01T04:19:13Z/2000-02-01T13:55:34Z
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, Chu comma You-Hua, 2001, 'The Luminous Giant HII Regions in M101', 1.0, European Space Agency, https://doi.org/10.5270/esa-gtn9pwl