Results 131 to 140 of about 37,027 (256)

Observations of CO in the Magellanic irregular galaxy NGC 55 [PDF]

open access: yes
The content of molecular gas in galaxies, mainly H2, is one of the key observations necessary for the understanding of star formation processes and history.
Dettmar, Ralf-Juergen   +1 more
core   +1 more source

Star Formation Histories of the LEGUS Dwarf Galaxies. II. Spatially Resolved Star Formation History of the Magellanic Irregular NGC 4449 [PDF]

open access: bronze, 2018
E Sacchi   +37 more
openalex   +1 more source

Emergence of the Galaxy Morphology–Star Formation Activity–Clustercentric Radius Relations in Galaxy Clusters

open access: yesThe Astrophysical Journal
We investigate when and how the relations of galaxy morphology and star-forming activity with clustercentric radius become evident in galaxy clusters. We identify 162 galaxy clusters with total mass ${{M}}_{\mathrm{tot}}^{\mathrm{cl}}\gt 5\times {10}^{13}
Sungwook E. Hong   +9 more
doaj   +1 more source

A Study of Two Dwarf Irregular Galaxies with AsymmetricalStar Formation Distributions [PDF]

open access: bronze, 2018
Deidre A. Hunter   +51 more
openalex   +1 more source

COSMIC-L: A Photometric Catalog of Observed Stars in the Large Magellanic Cloud

open access: yesThe Astrophysical Journal Supplement Series
The Magellanic Clouds are two nearby dwarf irregular galaxies, the study of which can help us in understanding galaxy and stellar evolution. In particular, the Large Magellanic Cloud, the larger one, contains approximately 30 billion stars at various ...
Antonio Franco   +3 more
doaj   +1 more source

Relationships between the Stellar, Gaseous, and Star Formation Disks in LITTLE THINGS Dwarf Irregular Galaxies: Indirect Evidence for Substantial Fractions of Dark Molecular Gas [PDF]

open access: bronze, 2021
Deidre A. Hunter   +9 more
openalex   +1 more source

NEAR-INFRARED PHOTOMETRY OF THE STAR CLUSTERS IN THE DWARF IRREGULAR GALAXY IC 5152 [PDF]

open access: bronze, 2006
Jaemann Kyeong   +4 more
openalex   +1 more source

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