activity
20022025
most citedFirst Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way

1.9k citations · 16.8k across the 67 of their papers we have counts for

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11 papers · 1 filter

astro-ph.SR2023★ 12 cited

A resolved rotating disk wind from a young T Tauri star in the Bok globule CB26

R. Launhardt, Ya. N. Pavlyuchenkov, V. V. Akimkin +9

The disk-outflow connection plays a key role in extracting excess angular momentum from a forming protostar. We have previously reported the discovery of a small molecular outflow…

astro-ph.SR2021★ 14 cited

An unbiased NOEMA 2.6 to 4 mm survey of the GG Tau ring: First detection of CCS in a protoplanetary disk

N. T. Phuong, A. Dutrey, E. Chapillon +13

Molecular line surveys are among the main tools to probe the structure and physical conditions in protoplanetary disks (PPDs), the birthplace of planets. The large radial and verti…

astro-ph.SR2020★ 24 cited

GG Tau A: gas properties and dynamics from the cavity to the outer disk

N. T. Phuong, A. Dutrey, P. N. Diep +13

We used new ALMA CO and CO(3-2) observations obtained at high angular resolution (0.2") together with previous CO(3-2) and (6-5) ALMA data and continuum maps at…

astro-ph.SR2019★ 105 cited

Masses and Implications for Ages of Low-Mass Pre-Main Sequence Stars in Taurus and Ophiuchus

M. Simon, S. Guilloteau, Tracy L. Beck +6

The accuracy of masses of pre-main sequence (PMS) stars derived from their locations on the Hertzsprung-Russell Diagram (HRD) can be tested by comparison with accurate and precise…

astro-ph.SR2017★ 65 cited

Dynamical Masses of Low Mass Stars in the Taurus and Ophiuchus Star Forming Regions

M. Simon, S. Guilloteau, E. di Folco +8

We report new dynamical masses for 5 pre-main sequence (PMS) stars in the L1495 region of the Taurus star-forming region (SFR) and 6 in the L1688 region of the Ophiuchus SFR. Since…

astro-ph.SR2016★ 48 cited

The hybrid disks: a search and study to better understand evolution of disks

J. Pericaud, E. Di Folco, A. Dutrey +2

The increased sensitivity of millimeter-wave facilities now makes possible the detection of low amounts of gas in debris disks. Some of the gas-rich debris disks harbor peculiar pr…