43 citations · 87 across the 7 of their papers we have counts for
7 papers
T CrA has a companion: First direct detection of T CrA B with VLTI/MATISSE
J. Varga, A. Matter, F. Millour +21
T CrA is a Herbig Ae-type young star in a complex circumstellar environment; it includes a circumstellar disk, accretion streamers, jets, and outflows. It has long been suspected t…
The hot corino-like chemistry of four FUor-like protostars
Fernando Cruz-Sáenz de Miera, Audrey Coutens, Ágnes Kóspál +3
Context: Compared to Class 0 protostars, the higher densities and lower temperatures of the disk midplanes of Class I young stellar objects (YSOs) limit the detectability of comple…
Gaia20bdk -- a new FUor in Sh 2-301 Star Forming Region
M. Siwak, Á. Kóspál, P. Ábrahám +28
Context. We analyse multi-colour photometric and spectroscopic observations of a Young Stellar Object Gaia20bdk. Aims. We aim to investigate the exact nature of the eruptive phenom…
Brightness and mass accretion rate evolution during the 2022 burst of EX~Lupi
F. Cruz-Sáenz de Miera, Á. Kóspál, P. Ábrahám +18
EX Lupi is the prototype by which EXor-type outbursts were defined. It has experienced multiple accretion-related bursts and outbursts throughout the last decades, whose study have…
94 Ceti: a triple star with a planet and dust disc
J. Wiegert, V. Faramaz, F. Cruz-Saenz de Miera
94 Ceti is a triple star system with a circumprimary gas giant planet and far-infrared excess. Such excesses around main sequence stars are likely due to debris discs, and are cons…
Deep LMT/AzTEC millimeter observations of Epsilon Eridani and its surroundings
M. Chavez-Dagostino, E. Bertone, F. Cruz-Saenz de Miera +21
Epsilon Eridani is a nearby, young Sun-like star that hosts a ring of cool debris analogous to the solar system's Edgeworth-Kuiper belt. Early observations at (sub-)mm wavelengths…
Lithium abundance in a sample of solar-like stars
R. López-Valdivia, J. B. Hernández-Águila, E. Bertone +3
We report on the determination of the lithium abundance [A(Li)] of 52 solar-like stars. For 41 objects the A(Li) here presented corresponds to the first measurement. We have measur…