Abundances and Density Structure of the Inner Circumstellar Ring Around SN 1987A
Accurate Stellar Population Studies from Multiband Photometric Observations
A New View of the Circumstellar Environment of SN 1987A
Hubble Space Telescope and Ground-based Observations of SN 1993J and SN 1998S: CNO Processing in the Progenitors
Hubble Space Telescope Observations of the Large Magellanic Cloud Field around SN 1987A: Distance Determination with Red Clump and Tip of the Red Giant Branch Stars
Infrared emission towards SN 1987A 11 years after outburst: Measurements with ISOCAM
Low-Mass Pre-Main-Sequence Stars in the Large Magellanic Cloud. III. Accretion Rates from Hubble Space Telescope WFPC2 Observations
Modelling supernova line profile asymmetries to determine ejecta dust masses: SN 1987A from days 714 to 3604
On the Emergence and Discovery of Hot Spots in SNR 1987A
Photometric Determination of the Mass Accretion Rates of Pre-main-sequence Stars. I. Method and Application to the SN 1987A Field
The Destruction of the Circumstellar Ring of SN 1987A
The late-time expansion of the ejecta of SN 1987A
The outer rings of SN 1987A
The Three-dimensional Circumstellar Environment of SN 1987A
X-ray illumination of the ejecta of supernova 1987A
Young Stellar Populations around SN 1987A
Instrument
FOS/BL, FOS/RD, WFPC2, WFPC2/PC
Temporal Coverage
1996-01-29T22:43:17Z/1996-09-24T00:49:46Z
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, Kirshner comma Robert P., 1997, 'SINS: Supernova INtensive Study - Cycle 5', 1.0, European Space Agency, https://doi.org/10.5270/esa-pu0ni2e