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19962024
most citedThe Star Formation Rate and Dense Molecular Gas in Galaxies

1k citations · 7k across the 138 of their papers we have counts for

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Showing 2022Show all

10 papers · 1 filter

astro-ph.GA2022★ 2 cited

Non-detection of Broad Hydrogen Radio Recombination Lines in Circinus Galaxy

Junzhi Wang, Yong Shi, Zhi-Yu Zhang +5

The line widths of broad line regions (BLRs) of AGNs are key parameters for understanding the central super massive black holes (SMBHs). However, due to obscuration from dusty toru…

astro-ph.GA2022★ 1 cited

A scaling relation in [C II]-detected galaxies and its likely application in cosmology

Y. Wu, Yu Gao, Jun-Feng Wang

We identify and investigate a possible correlation between the luminosity and linewidth in the -detected galaxies. Observationally, the strength of t…

astro-ph.GA2022★ 17 cited

The correlation between WISE 12 m emission and molecular gas tracers on sub-kpc scales in nearby star-forming galaxies

Yang Gao, Qing-Hua Tan, Yu Gao +4

We complement the MALATANG sample of dense gas in nearby galaxies with archival observations of and its isotopologues to determine scaling relations between Wide-fiel…

astro-ph.GA2022★ 9 cited

Dense Gas and Star Formation in Nearby Infrared Bright Galaxies: APEX survey of HCN and HCO+ J=2-1

Jing Zhou, Zhi-Yu Zhang, Yu Gao +6

Both Galactic and extragalactic studies on star formation suggest that stars form directly from dense molecular gas. To trace such high volume density gas, HCN and HCO+ J=1-0 have…

astro-ph.GA2022★ 11 cited

Distributed YSOs in the Perseus Molecular Cloud from the Gaia and LAMOST Surveys

Xiao-Long Wang, Min Fang, Yu Gao +5

Identifying the young optically visible population in a star-forming region is essential for fully understanding the star formation event. In this paper, We identify 211 candidate…

astro-ph.GA2022

Diagnosing deceivingly cold dusty galaxies at 3.5<z<6: a substantial population of compact starbursts with high infrared optical depths

Shuowen Jin, Emanuele Daddi, Georgios E. Magdis +9

Using NOEMA and ALMA 3mm line scans, we measure spectroscopic redshifts of six new dusty galaxies at 3.5<z<4.2 by solidly detecting [CI](1-0) and CO transitions. The sample was sel…