474 citations · 4.8k across the 91 of their papers we have counts for
87 papers
The EDGE-CALIFA Survey: Spatially Resolved 13CO(1-0) Observations and Variations in 12CO(1-0)/13CO(1-0) in Nearby Galaxies on kpc Scales
Yixian Cao, Tony Wong, Alberto D. Bolatto +12
We present 13CO(1-0) observations for the EDGE-CALIFA survey, which is a mapping survey of 126 nearby galaxies at a typical spatial resolution of 1.5 kpc. Using detected 12CO(1-0)…
Exploring the Impact of Galactic Interactions and Mergers on the Central Star Formation of APEX/EDGE-CALIFA Galaxies
Y. Garay-Solis, J. K. Barrera-Ballesteros, D. Colombo +5
Galactic interactions and subsequent mergers are a paramount channel for galaxy evolution. In this work, we use the data from 236 star forming CALIFA galaxies with integrated molec…
An Unbiased CO Survey Toward the Northern Region of the Small Magellanic Cloud with the Atacama Compact Array. II. CO Cloud Catalog
Takahiro Ohno, Kazuki Tokuda, Ayu Konishi +16
The nature of molecular clouds and their statistical behavior in subsolar metallicity environments are not fully explored yet. We analyzed data from an unbiased CO( = 2-1) surve…
The local and global relations between , and that regulate star-formation
Sebastián F. Sánchez, Daysi C. Gómez Medina, J. K. Barrera-Ballesteros +3
Star-formation is one of the main processes that shape galaxies, defining its stellar population and metallicity production and enrichment. It is nowadays known that this process i…
The Volumetric Star Formation Law in the Almost Edge-on Galaxy NGC 4302 Revealed by ALMA
Kijeong Yim, Tony Wong, Richard J. Rand
We observe the almost edge-on (i 90 degrees) galaxy NGC 4302 using ALMA (CO) and VLA (H I) to measure the gas disk thickness for investigating the volumetric star formation…
The EDGE-CALIFA survey: The role of spiral arms and bars in driving central molecular gas concentrations
Si-Yue Yu, Veselina Kalinova, Dario Colombo +9
Shocks and torques produced by non-axisymmetric structures such as spiral arms and bars may transport gas to galaxy central regions. We test this hypothesis by studying the depende…