activity
20092026
most citedX-Shooter spectroscopy of young stellar objects in Lupus: Accretion properties of class II and transitional objects

471 citations · 1.1k across the 21 of their papers we have counts for

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Showing 2024Show all

6 papers · 1 filter

astro-ph.EP2024★ 7 cited

Intermediate mass T Tauri disk masses and a comparison to their Herbig disk descendants

L. M. Stapper, M. R. Hogerheijde, E. F. van Dishoeck +3

The precursors of Herbig stars are called Intermediate Mass T Tauri (IMTT) stars, which have spectral types later than F, but stellar masses between 1.5 and 5 M_\odot, and will eve…

astro-ph.SR2024

Discovery of an accretion streamer and a slow wide-angle outflow around FU Orionis

A. S. Hales, A. Gupta, D. Ruiz-Rodriguez +10

We present ALMA 12-m, 7-m & Total Power (TP) Array observations of the FU Orionis outbursting system, covering spatial scales ranging from 160 to 25,000 au. The high-resolution int…

astro-ph.SR2024★ 13 cited

Anatomy of the Class I protostar L1489 IRS with NOEMA -- I. Disk, streamers, outflow(s) and bubbles at 3mm

M. Tanious, R. Le Gal, R. Neri +7

Over the past few years, chemical studies have revealed multiple structures in the vicinity of young stellar objects (YSOs). It has become evident that specific physical conditions…

astro-ph.GA2024

The SPHERE view of the Taurus star-forming region

A. Garufi, C. Ginski, R. G. van Holstein +31

The sample of planet-forming disks observed by high-contrast imaging campaigns over the last decade is mature enough to enable the demographical analysis of individual star-forming…

astro-ph.SR2024

The SPHERE view of the Orion star-forming region

P. -G. Valegard, C. Ginski, A. Derkink +17

We present SPHERE/IRDIS H-band data for a sample of 23 stars in the Orion Star forming region observed within the DESTINYS (Disk Evolution Study Through Imaging of Nearby Young Sta…

astro-ph.GA2024★ 1 cited

The SPHERE view of the Chamaeleon I star-forming region

C. Ginski, A. Garufi, M. Benisty +32

We used VLT/SPHERE to observe 20 systems in the Cha I cloud in polarized scattered light in the near-infrared. We combined the scattered light observations with existing literature…