activity
19982023
most citedThe Wavelength Dependence of Interstellar Extinction from 1.25 to 8.0 microns Using GLIMPSE Data

848 citations · 7.9k across the 67 of their papers we have counts for

collaborators

67 papers

astro-ph.GA2023★ 19 cited

Unveiling the formation of the massive DR21 ridge

L. Bonne, S. Bontemps, N. Schneider +10

We present new CO(1-0), CO(1-0), HCO(1-0) and HCO(1-0) maps from the IRAM 30m telescope, and a spectrally-resolved [CII] 158 m map observed with…

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★ 24 cited

The SOFIA FEEDBACK Legacy Survey: Dynamics and mass ejection in the bipolar HII region RCW 36

L. Bonne, N. Schneider, P. García +20

We present [CII] 158 m and [OI] 63 m observations of the bipolar HII region RCW 36 in the Vela C molecular cloud, obtained within the SOFIA legacy project FEEDBACK, which is…

astro-ph.GA2022★ 18 cited

The Magnetic Field in the Milky Way Filamentary Bone G47

Ian W. Stephens, Philip C. Myers, Catherine Zucker +21

Star formation primarily occurs in filaments where magnetic fields are expected to be dynamically important. The largest and densest filaments trace spiral structure within galaxie…

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…