A Comprehensive Archival Chandra Search for X-Ray Emission from Ultracompact Dwarf Galaxies
An ultra-compact dwarf around the Sombrero galaxy (M104): the nearest massive UCD
A Peculiar Galaxy Near M104
A Revised Parallel-sequence Morphological Classification of Galaxies: Structure and Formation of S0 and Spheroidal Galaxies
Density Dependence of the Mass Function of Globular Star Clusters in the Sombrero Galaxy and Its Dynamical Implications
Diamonds on the Hat: globular clusters in the Sombrero galaxy (M104)
Evidence for a Constant Initial Mass Function in Early-type Galaxies Based on Their X-Ray Binary Populations
Extending the baseline: Spitzer mid-infrared photometry of globular cluster systems in the Centaurus A and Sombrero Galaxies
Hubble Space Telescope ACS Wide-Field Photometry of the Sombrero Galaxy Globular Cluster System
Spectra of globular clusters in the Sombrero galaxy: evidence for spectroscopic metallicity bimodality
The impact of satellite trails on Hubble Space Telescope observations
The ubiquity and dual nature of ultra-compact dwarfs
The X-Ray Luminosity Function of Low-mass X-Ray Binaries in Early-type Galaxies, Their Metal-rich, and Metal-poor Globular Clusters
Tracing the Giant Outer Halo of the Mysterious Massive Disk Galaxy M104. I. Photometry of the Extended Globular Cluster Systems
X-ray Emission from the Sombrero Galaxy: Discrete Sources
Instrument
ACS, ACS/HRC, ACS/WFC
Temporal Coverage
2003-05-16T12:57:49Z/2003-06-14T13:34:27Z
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, Noll et al., 2003, 'Hubble Heritage Observations of the Sombrero Galaxy', 1.0, European Space Agency, https://doi.org/10.5270/esa-0dwj3at
