papers

Publications (13)

astro-ph.EP2015

Infrared study of transitional disks in Ophiuchus with Herschel

Isabel Rebollido, Bruno Merín, Álvaro Ribas +7

Context. Observations of nearby star-forming regions with the Herschel Space Observatory complement our view of the protoplanetary disks in Ophiuchus with information about the out…

astro-ph.IM2024

JASMINE: Near-Infrared Astrometry and Time Series Photometry Science

Daisuke Kawata, Hajime Kawahara, Naoteru Gouda +86

Japan Astrometry Satellite Mission for INfrared Exploration (JASMINE) is a planned M-class science space mission by the Institute of Space and Astronautical Science, the Japan Aero…

astro-ph.IM2024

Large Projects in Astronomy: An Indian Endeavour

Yogesh Wadadekar, Shriharsh Tendulkar, Sanjit Mitra +6

Policy Brief on "Large Projects in Astronomy: An Indian Endeavour", distilled from the corresponding panel that was part of the discussions during S20 Policy Webinar on Astroinform…

astro-ph.SR2011

Ruling out unresolved binaries in five transitional disks VLT/NACO: deep 2.12 and 1.75 μm narrow-band imaging

Silvia Vicente, Bruno Merın, Markus Hartung +8

Aims. We aim at detecting the presence of companions inside the inner hole/gap region of a sample of five well known transitional disks using spatially-resolved imaging in the near…

astro-ph.GA2021

The 800pc long tidal tails of the Hyades star cluster: Possible discovery of candidate epicyclic overdensities from an open star cluster

Tereza Jerabkova, Henri M. J. Boffin, Giacomo Beccari +3

The tidal tails of stellar clusters provide an important tool for studying the birth conditions of the clusters and their evolution, coupling, and interaction with the Galactic pot…

astro-ph.SR2010

A Spitzer c2d Legacy Survey to Identify and Characterize Disks with Inner Dust Holes

Bruno Merín, Joanna M. Brown, Isa Oliveira +17

Understanding how disks dissipate is essential to studies of planet formation. However, identifying exactly how dust and gas dissipates is complicated due to difficulty in finding…

astro-ph.IM2024

AstroInformatics: Recommendations for Global Cooperation

Ashish Mahabal, Pranav Sharma, Rana Adhikari +45

Policy Brief on "AstroInformatics, Recommendations for Global Collaboration", distilled from panel discussions during S20 Policy Webinar on Astroinformatics for Sustainable Develop…

astro-ph.GA2023

Finding the dispersing siblings of young open clusters. Dynamical traceback simulations using Gaia DR3

Eero Vaher, David Hobbs, Paul McMillan +1

Context. Stars tend to form in clusters, but many escape their birth clusters very early. Identifying the escaped members of clusters can inform us about the dissolution of star cl…

astro-ph.GA2022

Asymmetrical tidal tails of open star clusters: stars crossing their cluster's prah challenge Newtonian gravitation

Pavel Kroupa, Tereza Jerabkova, Ingo Thies +14

After their birth a significant fraction of all stars pass through the tidal threshold (prah) of their cluster of origin into the classical tidal tails. The asymmetry between the n…

astro-ph.SR2018

The outbursting protostar 2MASS~22352345+7517076 and its environment

Maria Kun, Peter Abraham, Jose Antonio Acosta Pulido +2

We studied the Class I protostar 2MASS 22352345+7517076 whose dramatic brightening between the IRAS, Akari, and WISE surveys was reported by Onozato et al. (2015). 2MASS 22352345+7…

astro-ph.GA2023

VISIONS: The VISTA Star Formation Atlas -- I. Survey overview

Stefan Meingast, João Alves, Hervé Bouy +37

VISIONS is an ESO public survey of five nearby (d < 500 pc) star-forming molecular cloud complexes that are canonically associated with the constellations of Chamaeleon, Corona Aus…

astro-ph.SR2017

A revised estimate of the distance to the clouds in the Chamaeleon complex using the Tycho-Gaia Astrometric Solution

Jordan Voirin, Carlo F. Manara, Timo Prusti

The determination of the distance to dark star-forming clouds is a key parameter to derive the properties of the cloud itself, and of its stellar content. This parameter is still l…

astro-ph2006

Long-term infrared variability of the UX Ori-type star SV Cep

Attila Juhasz, Timo Prusti, Peter Abraham +1

We investigate the long-term optical-infrared variability of SV Cep, and explain it in the context of an existing UX Ori (UXOR) model. A 25-month monitoring programme was completed…