activity
20162024
most citedDense Gas in the Outer Spiral Arm of M51

23 citations · 32 across the 6 of their papers we have counts for

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Showing astro-ph.GAShow all

6 papers · 1 filter

astro-ph.GA2024

Revealing hidden structures in the Zone of Avoidance -- a blind MeerKAT HI Survey of the Vela Supercluster

Sambatriniaina H. A. Rajohnson, Renée C. Kraan-Korteweg, Bradley S. Frank +7

We conducted the MeerKAT Vela Supercluster survey, named VelaHI, to bridge the gap between the Vela SARAO MeerKAT Galactic Plane Survey (VelaSMGPS, $-2^{\circ} \leq b \leq 1^…

astro-ph.GA2023

Neutral Hydrogen content of dwarf galaxies in different environments

Hui-Jie Hu, Qi Guo, Pablo Renard +5

Environments play an important role in galaxy formation and evolution, particularly in regulating the content of neutral gas. However, current HI surveys have limitations in their…

astro-ph.GA2023

AMUSE-antlia I: Nuclear X-ray properties of early-type galaxies in a dynamically young galaxy cluster

Zhensong Hu, Yuanyuan Su, Zhiyuan Li +14

To understand the formation and growth of supermassive black holes (SMBHs) and their co-evolution with host galaxies, it is essential to know the impact of environment on the activ…

astro-ph.GA20235 cited

MIGHTEE-\HI: Possible interactions with the galaxy NGC~895

Brenda Namumba, Javier Román, Jesus Falcon Barroso +29

The transformation and evolution of a galaxy is strongly influenced by interactions with its environment. Neutral hydrogen (\HI) is an excellent way to trace these interactions. He…

astro-ph.GA20224 cited

HIPASS study of southern ultradiffuse galaxies and low surface brightness galaxies

Yun-Fan Zhou, Chandreyee Sengupta, Yogesh Chandola +4

We present results from an HI counterpart search using the HI Parkes All Sky Survey (HIPASS) for a sample of low surface brightness galaxies (LSBGs) and ultradiffuse galaxies (UDGs…

astro-ph.GA201623 cited

Dense Gas in the Outer Spiral Arm of M51

Hao Chen, Jonathan Braine, Yu Gao +2

There is a linear relation between the mass of dense gas, traced by the HCN(1-0) luminosity, and the star formation rate (SFR), traced by the far-infrared luminosity. Recent observ…