activity
20182026
most citedPENELLOPE: the ESO data legacy program to complement the Hubble UV Legacy Library of Young Stars (ULLYSES) I. Survey presentation and accretion properties of Orion OB1 and -Orionis

76 citations · 330 across the 43 of their papers we have counts for

collaborators
Showing 2024Show all

9 papers · 1 filter

astro-ph.SR2024★ 10 cited

A New Look at Disk Winds and External Photoevaporation in the -Orionis Cluster

K. Maucó, C. F. Manara, A. Bayo +12

Disk winds play a crucial role in the evolution of protoplanetary disks. Typical conditions for star and planet formation are in regions with intermediate or strong UV radiation fi…

astro-ph.SR2024

Measurement of interstellar extinction for classical T Tauri stars using far-UV H2 line fluxes

B. Fuhrmeister, P. C. Schneider, Th. Sperling +3

Understanding the interstellar and potentially circumstellar extinction in the sight lines of classical T Tauri stars is an important ingredient for constructing reliable spectral…

astro-ph.SR2024★ 9 cited

A tell-tale tracer for externally irradiated protoplanetary disks: comparing the [CI] 8727 A line and ALMA observations in proplyds

Mari-Liis Aru, Karina Mauco, Carlo F. Manara +15

The evolution of protoplanetary disks in regions with massive OB stars is influenced by externally driven winds that deplete the outer parts of disks. These winds have previously b…

astro-ph.SR2024

Evidence for magnetic boundary layer accretion in RU Lup. A spectrophotometric analysis

A. Armeni, B. Stelzer, A. Frasca +9

The aim of this work is to characterize the accretion process of the classical T Tauri Star RU Lup. We studied optical high-resolution spectroscopic observations from CHIRON and ES…

astro-ph.SR2024

A Multi-wavelength, Multi-epoch Monitoring Campaign of Accretion Variability in T Tauri Stars from the ODYSSEUS Survey. III. Optical Spectra

John Wendeborn, Catherine C. Espaillat, Thanawuth Thanathibodee +20

Classical T Tauri Stars (CTTSs) are highly variable stars that possess gas- and dust-rich disks from which planets form. Much of their variability is driven by mass accretion from…

astro-ph.SR2024

FitteR for Accretion ProPErties of T Tauri stars (FRAPPE): A new approach to use Class III spectra to derive stellar and accretion properties

R. A. B. Claes, J. Campbell-White, C. F. Manara +10

Studies of the stellar and accretion properties of classical T Tauri stars (CTTS) require comparison with photospheric spectral templates. Here we aim at expanding the currently av…

astro-ph.SR2024

North-PHASE: Studying Periodicity, Hot Spots, Accretion Stability and Early Evolution in young stars in the northern hemisphere

A. Sicilia-Aguilar, R. S. Kahar, M. E. Pelayo-Baldárrago +17

We present the overview and first results from the North-PHASE Legacy Survey, which follows six young clusters for five years, using the 2 deg FoV of the JAST80 telescope from…

astro-ph.SR2024

PENELLOPE\,VI. -- Searching the PENELLOPE/UVES sample with spectro-astrometry: Two new microjets of Sz 103 and XX Cha

T. Sperling, J. Eislöffel, C. F. Manara +7

The main goal of this study is to screen the PENELLOPE/UVES targets for outflow activity and find microjets via spectro-astrometry in, e.g., the [OI]6300 line. In total, 34 T\,T…

astro-ph.SR2024

A survey for variable young stars with small telescopes: VIII -- Properties of 1687 Gaia selected members in 21 nearby clusters

Dirk Froebrich, Aleks Scholz, Justyn Campbell-White +60

The Hunting Outbursting Young Stars (HOYS) project performs long-term, optical, multi-filter, high cadence monitoring of 25 nearby young clusters and star forming regions. Utilisin…