activity
20002013
most citedPre-main sequence spectroscopic binaries suitable for VLTI observations

115 citations · 401 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2013★ 4 cited

The eclipsing binary TY CrA revisited: What near-IR light curves tell us

M. Vanko, M. Ammler-von Eiff, T. Pribulla +3

New photometric observations of the hierarchical eclipsing TY CrA system were taken in the optical with VYSOS6 and in the near-IR with SOFI and REMIR. They are the first observatio…

astro-ph.SR2012★ 58 cited

The DWARF project: Eclipsing binaries - precise clocks to discover exoplanets

T. Pribulla, M. Vaňko, M. Ammler - von Eiff +53

We present a new observational campaign, DWARF, aimed at detection of circumbinary extrasolar planets using the timing of the minima of low-mass eclipsing binaries. The observation…

astro-ph.SR2010★ 28 cited

Pre-Main Sequence stars in the star forming complex Sh 2-284

F. Cusano, V. Ripepi, J. M. Alcala +10

Located at the galactic anticenter, Sh 2-284 is a HII region which harbors several young open clusters; Dolidze 25, a rare metal poor (Z~0.004) young cluster, is one of these. Give…

astro-ph.SR2009★ 63 cited

Variability of the transitional T Tauri star T Chamaeleontis

E. Schisano, E. Covino, J. M. Alcala' +3

We characterize the physical properties of T Chamaeleontis, a transitional T Tauri star showing UX Ori-type variability, and of its associated disc, and probe possible effects of d…

astro-ph2008★ 94 cited

The Spitzer c2d Survey of Large, Nearby, Interstellar Clouds.X. The Chamaeleon II Pre-Main Sequence Population as Observed With IRAC and MIPS

Juan M. Alcala', Loredana Spezzi, Nicholas Chapman +9

We discuss the results from the combined IRAC and MIPS c2d Spitzer Legacy survey observations and complementary optical and near infrared data of the Chamaeleon II (Cha II) dark cl…

astro-ph2007★ 115 cited

Pre-main sequence spectroscopic binaries suitable for VLTI observations

E. W. Guenther, M. Esposito, R. Mundt +4

A severe problem of the research in star-formation is that the masses of young stars are almost always estimated only from evolutionary tracks. Since the tracks published by differ…