Atacama Compact Array observations of the pulsar-wind nebula of SNR 0540-69.3
Ejecta, Dust, and Synchrotron Radiation in SNR B0540-69.3: A More Crab-Like Remnant than the Crab
HST/WFPC2 observations of the LMC pulsar PSR B0540-69
Hubble Space Telescope Observations of Oxygen-rich Supernova Remnants in the Magellanic Clouds. III. WFPC2 Imaging of the Young, Crab-like Supernova Remnant SNR 0540-69.3
Kinematics, structure and abundances of supernova remnant 0540-69.3
Neutron Star Astronomy with the HST
Optical observations of the young supernova remnant SNR 0540-69.3 and its pulsar
Spectral evolution and polarization of variable structures in the pulsar wind nebula of PSR B0540-69.3
Supernova remnants as a probe of dust grains in the interstellar medium
The near-infrared detection of PSR B0540-69 and its nebula
The X-Ray Structure and Spectrum of the Pulsar Wind Nebula Surrounding PSR B0540-69.3
The young pulsar PSR B0540-69.3 and its synchrotron nebula in the optical and X-rays
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1999-10-17T03:49:13Z/1999-10-17T17:03:53Z
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, Morse et al., 2000, 'The Distribution of Heavy Elements in Supernova Ejecta', 1.0, European Space Agency, https://doi.org/10.5270/esa-ha81csr
