A Low-mass Main-sequence Star and Accretion Disk in the Very Faint X-Ray Transient M15 X-3
An Inverse Look at the Center of M15
Does M15 Possess an Intermediate-Mass Black Hole in Its Core?
The Discovery of a Very Faint X-Ray Transient in the Globular Cluster M15
The Dynamical Distance to M15: Estimates of the Clusters Age and Mass and of the Absolute Magnitude of Its RR Lyrae Stars
The Dynamical Mass-to-Light Ratio Profile and Distance of the Globular Cluster M15
The Luminous Erupting Dwarf Nova CV 1 in the Dense Globular Cluster M15
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
2002-04-05T00:11:16Z/2002-04-05T00:54:56Z
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, McNamara comma Bernard J., 2003, 'Getting to the Core of The Matter: The Inner Region of M15', 1.0, European Space Agency, https://doi.org/10.5270/esa-5bliwsx