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20182026
most citedOn the HI Content of MaNGA Major Merger Pairs

20 citations · 20 across the 8 of their papers we have counts for

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Showing astro-ph.GAShow all

7 papers · 1 filter

astro-ph.GA2026

Widespread Inflows Reveal Baryonic Cycling in Star-forming and Quiescent Galaxies

Hassen M. Yesuf, Ravi Joshi, Yuxuan Zou +8

Cool-gas inflows, required to sustain star formation, have been fundamental in simulations yet remained observationally elusive. Using DESI spectroscopy of ~30,000 galaxies, we ide…

astro-ph.GA2026

The Structural Abundance Crisis of Massive Galaxies in Current Cosmological Simulations

Hassen M. Yesuf, Connor Bottrell, Luis C. Ho +5

The internal structure of galaxies encodes the complex baryon cycle driven by gas accretion, star formation, and feedback, together with secular evolution and environmentally drive…

astro-ph.GA2026

The Narrow-Line Seyfert 1 Phenomenon: Accretion State Versus Host Galaxy Properties

Kaizheng Guo, Hassen M. Yesuf, Lei Hao +3

The physical origin of the narrow-line Seyfert 1 (NLS1) and broad-line Seyfert 1 (BLS1) dichotomy remains debated, with competing scenarios invoking host-galaxy evolution or intrin…

astro-ph.GA2026

Beyond Mass and Multiscale Environments: What Shapes Low Surface Brightness Galaxies? Evidence from MaNGA

Mengting Shen, Hassen M. Yesuf, Lei Hao +4

The origin of low surface brightness (LSB) galaxies remains a key open question in galaxy formation, reflecting the balance internal mechanisms and environmental influence. Using M…

astro-ph.GA2026

SDSS-IV MaNGA: Distinct Structural Growth and Star Formation in Low and High Surface Brightness Disks

Mengting Shen, Jun Yin, Hassen M. Yesuf +7

We analyze a clean sample of 1,118 late-type, face-on galaxies without AGN contamination from the MaNGA survey. Their photometric structures are quantified via two-component (bulge…

astro-ph.GA2022★ 20 cited

On the HI Content of MaNGA Major Merger Pairs

Qingzheng Yu, Taotao Fang, Shuai Feng +4

The role of HI content in galaxy interactions is still under debate. To study the HI content of galaxy pairs at different merging stages, we compile a sample of 66 major-merger gal…