A binary origin for `blue stragglers in globular clusters
Addendum: Hubble Space Telescope Evidence for an Intermediate-Mass Black Hole in the Globular Cluster M15. II. Kinematic Analysis and Dynamical Modeling Astron. J. 124, 3270 (2002)
A homogeneous set of globular cluster relative distances and reddenings
A low-mass triple system with a wide L/T transition brown dwarf component: NLTT 51469AB/SDSS 2131-0119
An Inverse Look at the Center of M15
Characterizing the Adaptive Optics Off-Axis Point-Spread Function. II. Methods for Use in Laser Guide Star Observations
Crowded Field Photometry of M15 Using the TRIFFID Camera
Galactic Globular Cluster Relative Ages
Globular Cluster Photometry with the Hubble Space Telescope. VII. Color Gradients and Blue Stragglers in the Central Region of M30 from Wide Field Planetary Camera 2 Observations
Globular Cluster Photometry With the Hubble Space Telescope. V. WFPC Study of M15s Central density Cusp
Green Bank Telescope Discovery of Two Binary Millisecond Pulsars in the Globular Cluster M30
High-resolution optical imaging of the core of the globular cluster M15 with FastCam
HST color-magnitude diagrams of 74 galactic globular clusters in the HST F439W and F555W bands
Hubble Space Telescope Evidence for an Intermediate-Mass Black Hole in the Globular Cluster M15. II. Kinematic Analysis and Dynamical Modeling
Hubble Space Telescope Evidence for an Intermediate-Mass Black Hole in the Globular Cluster M15. I. STIS Spectroscopy and WFPC2 Photometry
Isochrone fitting of Galactic globular clusters - III. NGC 288, NGC 362, and NGC 6218 (M12)
Multi-epoch observations with high spatial resolution of multiple T Tauri systems
Multivariate analysis of globular cluster horizontal branch morphology: searching for the second parameter
On the Central Structure of M15
Proper-motion Membership Tests for Four Planetary Nebulae in Galactic Globular Clusters
Radial Color Gradient and Main-Sequence Mass Segregation in M30 (NGC 7099)
Revealing Probable Universal Features in the Lower Red Giant Branch Luminosity Functions of Galactic Globular Clusters
Serendipitous Discovery of a Cataclysmic Variable in the Globular Cluster NGC 6624
The ACS Survey of Galactic Globular Clusters. VIII. Effects of Environment on Globular Cluster Global Mass Functions
The Discovery of an Erupting Dwarf Nova in NGC 6624
The Discovery of a Second Luminous Low-Mass X-Ray Binary in the Globular Cluster M15
The initial helium abundance of the Galactic globular cluster system
The Luminous Erupting Dwarf Nova CV 1 in the Dense Globular Cluster M15
The Red Giant Branch luminosity function bump
The treatment of mixing in core helium burning models - II. Constraints from cluster star counts
Towards 21st century stellar models: Star clusters, supercomputing and asteroseismology
TRIFFID Photometry of Globular Cluster Cores - I. Photometric Techniques and Variable Stars in M15
Uncloaking Globular Clusters in the Inner Galaxy
Unveiling the Core of the Globular Cluster M15 in the Ultraviolet
UVES analysis of red giants in the bulge globular cluster NGC 6522
WFPC2 Observations of the Globular Cluster M30
Why hot horizontal branch stars can appear redder than red giants
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1994-03-31T04:50:17Z/1994-04-17T23:16:37Z
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.
