activity
20022026
most citedOptical and Infrared Spectroscopy of SN 1999ee and SN 1999ex

184 citations · 1.8k across the 60 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

37 papers · 1 filter

astro-ph.SR2026

HD 152384: A 5 Myr old debris disk system showing a gaseous ring of refractory elements at the dust sublimation radius

Mario van den Ancker, Daniela Iglesias, Olja Panić +2

Context: Circumstellar gas around young stars provides key insights into planet formation and disk evolution. HD 152384, a young (5 Myr) A0 V star in Sco-Cen, shows hybrid-disk tra…

astro-ph.SR2025

Coordinated Space- and Ground-based Monitoring of Accretion Bursts in a Protoplanetary Disk: The Orbital and Accretion Properties of DQ Tau

Hala Alqubelat, Carlo F. Manara, Justyn Campbell-White +9

Multiplicity in pre-main-sequence (PMS) systems shapes circumstellar and circumbinary disks, often producing features such as inner cavities, spiral arms, and gas streamers that fa…

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.SR2023★ 10 cited

Empirical Determination of the Lithium 6707.856 Å Wavelength in Young Stars

Justyn Campbell-White, Carlo F. Manara, Aurora Sicilia-Aguilar +20

Absorption features in stellar atmospheres are often used to calibrate photocentric velocities for kinematic analysis of further spectral lines. The Li feature at 6708 Å is…

astro-ph.SR2022★ 10 cited

X-Shooter Survey of Young Intermediate Mass Stars -- I. Stellar Characterization and Disc Evolution

Daniela P. Iglesias, Olja Panić, Mario van den Ancker +6

Intermediate mass stars (IMSs) represent the link between low-mass and high-mass stars and cover a key mass range for giant planet formation. In this paper, we present a spectrosco…

astro-ph.SR2022★ 21 cited

PENELLOPE III. The peculiar accretion variability of XX Cha and its impact on the observed spread of accretion rates

R. A. B. Claes, C. F. Manara, R. Garcia-Lopez +17

The processes regulating protoplanetary disk evolution are constrained by studying how mass accretion rates scale with stellar and disk properties. The spread in these relations ca…

astro-ph.SR2021★ 5 cited

First detection of a disk free of volatile elements around a young A-type star: A sign of collisions between rocky planets?

M. E. van den Ancker, N. P. Gentile Fusillo, T. J. Haworth +7

Aims. We present the first detailed analysis of the astrophysical parameters of the poorly studied Sco-Cen member HD 152384 and its circumstellar environment. Methods. We analyze n…

astro-ph.SR2020

Planet formation in intermediate-separation binary systems

O. Panić, T. J. Haworth, M. G. Petr-Gotzens +13

We report the first characterisation of the individual discs in the intermediate separation binary systems KK Oph and HD 144668 at millimetre wavelengths. In both systems the circu…

astro-ph.SR2020★ 15 cited

Statistics of wide pre-main sequence binaries in the Orion OB1 association

Andrei Tokovinin, Monika Petr-Gotzens, Cesar Briceno

Statistics of low-mass pre-main sequence binaries in the Orion OB1 association with separations ranging from 0.6" to 20" (220 to 7400 au at 370 pc) are studied using images from th…

astro-ph.SR2020★ 19 cited

The VMC Survey -- XXXVII. Pulsation periods of dust enshrouded AGB stars in the Magellanic Clouds

M. A. T. Groenewegen, A. Nanni, M. -R. L. Cioni +9

(abridged)Variability is a key property of stars on the asymptotic giant branch (AGB). Their pulsation period is related to the luminosity and mass-loss rate of the star. The long-…

astro-ph.SR2020★ 6 cited

The VMC survey -- XXXVI. Young stellar variability in the Large Magellanic Cloud

Viktor Zivkov, Joana M. Oliveira, Monika G. Petr-Gotzens +11

Studies of young stellar objects (YSOs) in the Galaxy have found that a significant fraction exhibit photometric variability. However, no systematic investigation has been conducte…

astro-ph.SR2019★ 54 cited

When the tale comes true: multiple populations and wide binaries in the Orion Nebula Cluster

Tereza Jerabkova, Giacomo Beccari, Henri M. J. Boffin +5

The high-quality OmegaCAM photometry of the 3x3 deg around the Orion Nebula Cluster (ONC) in r, and i filters by Beccari et al.(2017) revealed three well-separated pre-main sequenc…

astro-ph.SR2019★ 29 cited

System IMF of the 25 Ori Group from Planetary-Mass Objects to Intermediate/High-Mass Stars

Genaro Suárez, Juan José Downes, Carlos Román-Zúñiga +4

The stellar initial mass function (IMF) is an essential input for many astrophysical studies but only in a few cases it has been determined over the whole cluster mass range, limit…

astro-ph.SR2018★ 9 cited

Weak Magnetic Fields in Two Herbig Ae Systems: The SB2 AK Sco and the Presumed Binary HD 95881

S. P. Järvinen, T. A. Carroll, S. Hubrig +9

We report the detection of weak mean longitudinal magnetic fields in the Herbig Ae double-lined spectroscopic binary AK Sco and in the presumed spectroscopic Herbig Ae binary HD958…

astro-ph.SR2017★ 83 cited

A Tale of Three Cities: OmegaCAM discovers multiple sequences in the color-magnitude diagram of the Orion Nebula Cluster

G. Beccari, M. G. Petr-Gotzens, H. M. J. Boffin +15

As part of the Accretion Discs in H with OmegaCAM (ADHOC) survey, we imaged in r, i and H-alpha a region of 12x8 square degrees around the Orion Nebula Cluster. Thanks to the hi…

astro-ph.SR2017★ 22 cited

New Low-Mass Stars in the 25 Orionis Stellar Group and Orion OB1a Sub-association from SDSS-III/BOSS Spectroscopy

Genaro Suárez, Juan José Downes, Carlos Román-Zúñiga +6

The Orion OB1a sub-association is a rich low mass star (LMS) region. Previous spectroscopic studies have confirmed 160 LMSs in the 25 Orionis stellar group (25 Ori), which is the m…

astro-ph.SR2016★ 17 cited

Spectroscopic signatures of magnetospheric accretion in Herbig Ae/Be stars. I. The case of HD101412

M. Schöller, M. A. Pogodin, J. A. Cahuasqui +10

Models of magnetically-driven accretion and outflows reproduce many observational properties of T Tauri stars. This concept is not well established for the more massive Herbig Ae/B…

astro-ph.SR2015★ 10 cited

The frequency of accretion disks around single stars: Chamaeleon I

Sebastian Daemgen, R. Elliot Meyer, Ray Jayawardhana +1

It is well known that stellar companions can influence the evolution of a protoplanetary disk. Nevertheless, previous disk surveys did not - and could not - consistently exclude bi…

astro-ph.SR2015★ 22 cited

The VISTA Carina Nebula Survey II. Spatial distribution of the infrared-excess-selected young stellar population

Peter Zeidler, Thomas Preibisch, Thorsten Ratzka +2

We performed a deep wide-field (6.76 deg^2) near-infrared survey with the VISTA telescope that covers the entire extent of the Carina nebula complex (CNC). The point-source catalog…

astro-ph.SR2015

Protoplanetary Disk Evolution: Singles vs. Binaries

Sebastian Daemgen, Ray Jayawardhana, Monika G. Petr-Gotzens +1

Based on a large number of observations carried out in the last decade it appears that the fraction of stars with protoplanetary disks declines steadily between ~1 Myr and ~10 Myr.…

astro-ph.SR2015★ 28 cited

The VISTA Orion mini-survey: star formation in the Lynds 1630 North cloud

L. Spezzi, M. G. Petr-Gotzens, J. M. Alcalá +4

The Orion cloud complex presents a variety of star formation mechanisms and properties and it is still one of the most intriguing targets for star formation studies. We present VIS…

astro-ph.SR2015

The number fraction of discs around brown dwarfs in Orion OB1a and the 25 Orionis group

Juan José Downes, Carlos Román-Zúñiga, Javier Ballesteros-Paredes +7

We present a study of 15 new brown dwarfs belonging to the Myr old 25 Orionis group and Orion OB1a sub-association with spectral types between M6 and M9 and estimated masse…

astro-ph.SR2014

Probing the Structure of the Accretion Region in a Sample of Magnetic Herbig Ae/Be Stars

M. A. Pogodin, J. A. Cahuasqui, N. A. Drake +10

We present the results of a study of the temporal behaviour of several diagnostic lines formed in the region of the accretion-disk/star interaction in the three magnetic Herbig Ae…

astro-ph.SR2014★ 30 cited

The low mass star and sub-stellar populations of the 25 Orionis group

Juan José Downes, César Briceño, Cecilia Mateu +6

We present the results of a survey of the low mass star and brown dwarf population of the 25 Orionis group. Using optical photometry from the CIDA Deep Survey of Orion, near IR pho…