activity
20062025
most citedVOSA: Virtual Observatory SED Analyzer. An application to the Collinder 69 open cluster

604 citations · 4.1k across the 56 of their papers we have counts for

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Showing astro-ph.SRShow all

26 papers · 1 filter

astro-ph.SR2024

Substellar candidates at the earliest stages: the SUCANES database

A. M. Pérez-García, N. Huélamo, A. García-López +11

Brown dwarfs are the bridge between low-mass stars and giant planets. One way of shedding light on their dominant formation mechanism is to study them at the earliest stages of the…

astro-ph.SR2022★ 109 cited

MINDS. The detection of CO with JWST-MIRI indicates abundant CO in a protoplanetary disk

Sierra L. Grant, Ewine F. van Dishoeck, Benoît Tabone +43

We present JWST-MIRI MRS spectra of the protoplanetary disk around the low-mass T Tauri star GW Lup from the MIRI mid-INfrared Disk Survey (MINDS) GTO program. Emission from $^{12}…

astro-ph.SR2020★ 16 cited

Ultracool Dwarfs in deep extragalactic surveys using the Virtual Observatory: ALHAMBRA and COSMOS

E. Solano, M. C. Gálvez-Ortiz, E. L. Martín +8

Ultracool dwarfs encompass a wide variety of compact stellar-like objects with spectra classified as late-M, L, T and Y. Most of them have been discovered using wide-field imaging…

astro-ph.SR2018★ 33 cited

A multi-wavelength view of magnetic flaring from PMS stars

E. Flaccomio, G. Micela, S. Sciortino +5

Flares from the Sun and other stars are most prominently observed in the soft X-ray band. Most of the radiated energy, however, is released at optical/UV wavelengths. In spite of d…

astro-ph.SR2016★ 17 cited

Physical parameters of late M-type members of Chamaleon I and TW Hydrae Association: Dust settling, age dispersion and activity

A. Bayo, D. Barrado, F. Allard +6

Although mid-to-late type M dwarfs are the most common stars in our stellar neighborhood, our knowledge of these objects is still limited. Open questions include the evolution of t…

astro-ph.SR2016★ 22 cited

A Model for (Quasi-)Periodic Multi-wavelength Photometric Variability in Young Stellar Objects

Aurora Y. Kesseli, Maya A. Petkova, Kenneth Wood +7

We present radiation transfer models of rotating young stellar objects (YSOs) with hotspots in their atmospheres, inner disk warps and other 3-D effects in the nearby circumstellar…