A Hubble Space Telescope Survey for Novae in M87. I. Light and Color Curves, Spatial Distributions, and the Nova Rate
An X-ray view of 82 LINERs with Chandra and XMM-Newton data
Doppler boosting, superluminal motion, and the kinematics of AGN jets
Flaring X-Ray Emission from HST-1, a Knot in the M87 Jet
Hubble Space Telescope Observations of Superluminal Motion in the M87 Jet
Internal structure and dynamics of the kiloparsec-scale jet in M87
Low optical polarization at the core of the optically thin jet of M87
Milliarcsecond-Scale Spectral Properties and Jet Motions in M 87
The Event Horizon of M87
The metallicity distribution function of globular clusters systems through near-infrared photometry
The Optical-Near-Infrared Spectrum of the M87 Jet fromHubble Space Telescope Observations
The Outburst of HST-1 in the M87 Jet
The synchrotron spectrum of the M87 jet
The X-Ray Emissions from the M87 Jet: Diagnostics and Physical Interpretation
X-ray nature of the LINER nuclear sources
Instrument
FOC/96, WFPC2, WFPC2/PC
Temporal Coverage
1996-07-31T01:21:28Z/1998-02-25T16:26:53Z
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, Biretta comma John A., 1999, 'Secular Changes in the Jet of M87', 1.0, European Space Agency, https://doi.org/10.5270/esa-y7ns8dm