output
20042026
most citedThe Gaia mission

7.1k citations

Showing 2023 · astro-ph.GAShow all

9 papers · 2 filters

astro-ph.GA20239 cited

UV-Bright Star-Forming Clumps and Their Host Galaxies in UVCANDELS at 0.5 z 1

Alec Martin, Yicheng Guo, Xin Wang +32

Giant star-forming clumps are a prominent feature of star-forming galaxies (SFGs) and contain important clues on galaxy formation and evolution. However, basic demographics of clum…

astro-ph.GA20232 cited

Zwicky Transient Facility and Globular Clusters: the gr-Band Period-Luminosity Relations for Mira Variables at Maximum Light and Their Applications to Local Galaxies

Chow-Choong Ngeow, Jia-Yu Ou, Anupam Bhardwaj +3

Based on 14 Miras located in 7 globular clusters, we derived the first gr-band period-luminosity (PL) at maximum light for the large-amplitude Mira variables using the multi-year l…

astro-ph.GA202311 cited

A Tale of 3 Dwarfs: No Extreme Cluster Formation in Extreme Star-Forming Galaxies

Rupali Chandar, Miranda Caputo, Angus Mok +8

Nearly all current simulations predict that outcomes of the star formation process, such as the fraction of stars that form in bound clusters (Gamma), depend on the intensity of st…

astro-ph.GA202311 cited

Early results from GLASS-JWST. XX: Unveiling a population of "red-excess'' galaxies in Abell2744 and in the coeval field

Benedetta Vulcani, Tommaso Treu, Antonello Calabro +26

We combine JWST/NIRCam imaging and MUSE data to characterize the properties of galaxies in different environmental conditions in the cluster Abell2744 () and in its immed…

astro-ph.GA20234 cited

Surveying the Giant HII Regions of the Milky Way with SOFIA: V. DR7 and K3-50

James M. De Buizer, Wanggi Lim, James T. Radomski +1

We present our fifth set of results from our mid-infrared imaging survey of Milky Way Giant HII (GHII) regions with our detailed analysis of DR7 and K3-50. We obtained 20/25 and 37…

astro-ph.GA20236 cited

Molecular gas in super spiral galaxies

Ute Lisenfeld, Patrick M. Ogle, Philip N. Appleton +2

At the highest stellar masses (log(\mstar) 11.5 \msun), only a small fraction of galaxies are disk-like and actively star-forming objects. These so-called `super spirals'…