activity
20082026
most citedA Steeper than Linear Disk Mass-Stellar Mass Scaling Relation

455 citations · 2.3k across the 68 of their papers we have counts for

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Showing 2020Show all

6 papers · 1 filter

astro-ph.EP2020★ 5 cited

Debris discs in binaries: morphology and photometric signatures

Philippe Thebault, Quentin Kral, Johan Olofsson

We aim to see whether debris belts evolving in between two stars may be impacted by the presence of the companion and whether this leaves any detectable signature that could be obs…

astro-ph.SR2020

Search for associations containing young stars (SACY) VIII. An updated census of spectroscopic binary systems showing hints of non-universal multiplicity among these associations

S. Zúñiga-Fernández, A. Bayo, P. Elliott +10

We seek to update the spectroscopy binary fraction of the SACY (Search for Associations Containing Young stars) sample taking in consideration all possible biases in our identifica…

astro-ph.EP2020

Dust trapping around Lagrangian points in protoplanetary disks

Matias Montesinos, Juan Garrido-Deutelmoser, Johan Olofsson +5

Trojans are defined as objects that share the orbit of a planet at the stable Lagrangian points and . In the Solar System, these bodies show a broad size distribution ra…

astro-ph.SR2020★ 33 cited

The challenge of measuring the phase function of debris disks. Application to HR\,4796

J. Olofsson, J. Milli, A. Bayo +2

Abridged: Debris disks are valuable systems to study dust properties. Because they are optically thin at all wavelengths, we have direct access to the properties of dust grains. On…

astro-ph.SR2020

Exocomets: A spectroscopic survey

I. Rebollido, C. Eiroa, B. Montesinos +18

While exoplanets are now routinely detected, the detection of small bodies in extrasolar systems remains challenging. Since the discovery of sporadic events interpreted as exocomet…

astro-ph.EP2020

ISPY -- NACO Imaging Survey for Planets around Young stars: Survey description and results from the first 2.5 years of observations

R. Launhardt, Th. Henning, A. Quirrenbach +21

The occurrence rate of long-period giant planets around young stars is highly uncertain since it is not only governed by the protoplanetary disc structure and planet formation proc…