activity
20122023
most citedChemistry in Infrared Dark Cloud Clumps: a Molecular Line Survey at 3 mm

213 citations · 905 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.GA2023★ 68 cited

The ALMA Survey of 70 m Dark High-mass Clumps in Early Stages (ASHES). IX. Physical Properties and Spatial Distribution of Cores in IRDCs

Kaho Morii, Patricio Sanhueza, Fumitaka Nakamura +13

The initial conditions found in infrared dark clouds (IRDCs) provide insights on how high-mass stars and stellar clusters form. We have conducted high-angular resolution and high-s…

astro-ph.GA2022★ 28 cited

The ALMA Survey of 70 Dark High-mass Clumps in Early Stages (ASHES). VII: Chemistry of Embedded Dense Cores

Shanghuo Li, Patricio Sanhueza, Xing Lu +15

We present a study of chemistry toward 294 dense cores in 12 molecular clumps using the data obtained from the ALMA Survey of 70 dark High-mass clumps in Early Stages (ASH…

astro-ph.GA2021★ 27 cited

The ALMA Survey of 70 m Dark High-mass Clumps in Early Stages (ASHES). V. Deuterated Molecules in the 70 m dark IRDC G14.492-00.139

Takeshi Sakai, Patricio Sanhueza, Kenji Furuya +14

We have observed the 70 m dark infrared dark cloud (IRDC) G14.492-00.139 in the ND =3--2, DCO =3--2, DCN =3--2, and CO =2--1 lines, using the Atac…

astro-ph.GA2021★ 41 cited

The ALMA Survey of 70 m Dark High-mass Clumps in Early Stages (ASHES). IV. Star formation signatures in G023.477

Kaho Morii, Patricio Sanhueza, Fumitaka Nakamura +15

With a mass of 1000 and a surface density of 0.5 g cm, G023.477+0.114 also known as IRDC 18310-4 is an infrared dark cloud (IRDC) that has the potentia…

astro-ph.GA2021★ 100 cited

Gravity Driven Magnetic Field at ~1000 au Scales in High-mass Star Formation

Patricio Sanhueza, Josep Miquel Girart, Marco Padovani +20

A full understanding of high-mass star formation requires the study of one of the most elusive components of the energy balance in the interstellar medium: magnetic fields. We repo…

astro-ph.GA2021★ 22 cited

The ALMA Survey of 70m Dark High-mass Clumps in Early Stages (ASHES) III. A Young Molecular Outflow Driven by a Decelerating Jet

Daniel Tafoya, Patricio Sanhueza, Qizhou Zhang +12

We present a spatio-kinematical analysis of the CO~(=21) line emission, observed with the Atacama Large Millimter/submillimter Array (ALMA), of the outflow associat…

astro-ph.GA2021★ 39 cited

Digging into the Interior of Hot Cores with ALMA (DIHCA). I. Dissecting the High-mass Star-Forming Core G335.579-0.292 MM1

Fernando A. Olguin, Patricio Sanhueza, Andrés E. Guzmán +10

We observed the high-mass star-forming region G335.579-0.292 with the Atacama Large Millimeter/submillimeter Array (ALMA) at 226 GHz with an angular resolution of 0.3'' ($\sim 1000…

astro-ph.GA2021★ 38 cited

Galaxy mergers up to z < 2.5 II: AGN incidence of merging galaxies at separations of 3-15 kpc

Andrea Silva, Danilo Marchesini, John D. Silverman +4

We present a study of the incidence of active galactic nucleus (AGN) in a sample of major merging systems at 0.3<z<2.5. Galaxies in this merger sample have projected separations be…

astro-ph.GA2020★ 11 cited

Observations of the [CI] (-) emission toward the massive star-forming region RCW38: further evidence for highly-clumped density distribution of the molecular gas

Natsuko Izumi, Yasuo Fukui, Kengo Tachihara +14

We present observations of the - fine-structure line of atomic carbon using the ASTE 10 m sub-mm telescope towards RCW38, the youngest super star cluster in the Milky…

astro-ph.GA2020★ 62 cited

The ALMA Survey of 70 Dark High-mass Clumps in Early Stages (ASHES). II: Molecular Outflows in the Extreme Early Stages of Protocluster Formation

Shanghuo Li, Patricio Sanhueza, Qizhou Zhang +15

We present a study of outflows at extremely early stages of high-mass star formation obtained from the ALMA Survey of 70 dark High-mass clumps in Early Stages (ASHES). Twe…

astro-ph.GA2019★ 207 cited

The ALMA Survey of 70 m dark High-mass clumps in Early Stages (ASHES). I. Pilot Survey: Clump Fragmentation

Patricio Sanhueza, Yanett Contreras, Benjamin Wu +20

(Abridged) ASHES has been designed to systematically characterize the earliest stages and to constrain theories of high-mass star formation. A total of 12 massive (>500 …

astro-ph.GA2018★ 34 cited

Galaxy mergers up to z<2.5 I : The star formation properties of merging galaxies at separations 3-15 kpc

Andrea Silva, Danilo Marchesini, John D. Silverman +7

We present a study of the influence of galaxy mergers on star formation at 0.3<z<2.5. Major mergers are selected from the CANDELS/3D-HST catalog using a peak-finding algorithm. Mer…

astro-ph.GA2017★ 15 cited

SMA Observations of the Hot Molecular Core IRAS 18566+0408

Andrea Silva, Qizhou Zhang, Patricio Sanhueza +6

We present Submillimeter Array (SMA) observations toward the high-mass star-forming region IRAS 18566+0408. Observations at 1.3 mm continuum and in several molecular line transitio…

astro-ph.GA2012★ 213 cited

Chemistry in Infrared Dark Cloud Clumps: a Molecular Line Survey at 3 mm

Patricio Sanhueza, James M. Jackson, Jonathan B. Foster +3

We have observed 37 Infrared Dark Clouds (IRDCs), containing a total of 159 clumps, in high-density molecular tracers at 3 mm using the 22-meter ATNF Mopra Telescope located in Aus…