148 papers found
Refreshing results…
A Global Star-Forming Episode in M31 2–4 Gyr Ago
The Panchromatichubbleandromeda Treasury. Xi. The Spatially Resolved Recent Star Formation History of M31
The link between mass distribution and starbursts in dwarf galaxies★
The Star Formation Histories of Local Group Dwarf Galaxies. Iii. Characterizing Quenching in Low-Mass Galaxies
Characterizing the Star Formation of the Low-Mass Shield Galaxies Fromhubble Space Telescopeimaging
The SHIELD Multi-Wavelength Archive
The Panchromatic Hubble Andromeda Treasury Survey: UV-IR Photometry of 117 Million Stars
Escape fraction of ionizing photons from a dwarf galaxy NGC 4214
The Panchromatic Hubble Andromeda Treasury. Progression of Large-Scale Star Formation Across Space and Time in M 31
The Panchromatic Hubble Andromeda Treasury. X. Ultraviolet to Infrared Photometry of 117 Million Equidistant Stars
The Supernova Progenitor Mass Distributions of M31 and M33: Further Evidence for an Upper Mass Limit
Delayed Star Formation in Isolated Dwarf Galaxies:hubble Space Telescopestar Formation History of the Aquarius Dwarf Irregular
Supplementary Online Material for Article, "THE PANCHROMATIC HUBBLE ANDROMEDA TREASURY. X. ULTRAVIOLET TO INFRARED PHOTOMETRY OF 117 MILLION EQUIDISTANT STARS"
Constraints for the Progenitor Masses of 17 Historic Core-Collapse Supernovae
The Panchromatic Hubble Andromeda Treasury. Progression of Large-Scale Star Formation across Space and Time in M31
Evolution of Thermally Pulsing Asymptotic Giant Branch Stars. Iv. Constraining Mass Loss and Lifetimes of Low Mass, Low Metallicity Agb Stars
The Star Formation Histories of Local Group Dwarf Galaxies. I.HUBBLE Space Telescope/Wide Field Planetary Camera 2 Observations
The Star Formation Histories of Local Group Dwarf Galaxies. Ii. Searching for Signatures of Reionization
Comparing M31 and Milky Way Satellites: The Extended Star Formation Histories of Andromeda Ii and Andromeda Xvi
The Panchromatic Hubble Andromeda Treasury. Vi. The Reliability of Far-Ultraviolet Flux as a Star Formation Tracer on Subkiloparsec Scales
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