activity
20052020
most citedNPARSEC: NTT Parallaxes of Southern Extremely Cool objects. Goals, targets, procedures and first results

65 citations · 111 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2020★ 11 cited

A new look at Sco OB1 association with Gaia DR2

L. Yalyalieva, G. Carraro, R. Vazquez +3

We present and discuss photometric optical data in the area of the OB association Sco OB1 covering about 1 squared degree. UBVI photometry is employed in tandem with Gaia DR2 data…

astro-ph.SR2016★ 9 cited

Stellar populations in the Carina region: The Galactic plane at l = 291

J. A. Molina-Lera, G. Baume, R. Gamen +2

Previous studies of the Carina region have revealed its complexity and richness as well as a significant number of early-type stars. In many cases, these studies only concentrated…

astro-ph.GA2015★ 8 cited

Insights into the properties of the Local (Orion) spiral arm. NGC 2302: First results and description of the program

E. Costa, A. Moitinho, M. Radiszc +4

The spiral structure of the Milky Way is highly uncertain and is the subject of much discussion nowadays. We present the first result from a program that determines the properties…

astro-ph.SR2013★ 65 cited

NPARSEC: NTT Parallaxes of Southern Extremely Cool objects. Goals, targets, procedures and first results

R. L. Smart, C. G. Tinney, B. Bucciarelli +21

The discovery and subsequent detailed study of T dwarfs has provided many surprises and pushed the physics and modeling of cool atmospheres in unpredicted directions. Distance is a…

astro-ph.GA2012★ 1 cited

Stellar populations in the surrounding field of the LMC clusters NGC 2154 and NGC 1898

E. Chiosi, G. Baume, G. Carraro +2

In this paper we present a study and comparison of the star formation rates (SFR) in the fields around NGC 1898 and NGC 2154, two intermediate-age star clusters located in very dif…

astro-ph2005★ 17 cited

Three active M dwarfs within 8 pc: L 449-1, L 43-72, & LP 949-15

R. -D. Scholz, G. Lo Curto, R. A. Méndez +4

Three nearby star candidates were selected as bright 2MASS point sources without associated optical sources, i.e. with potentially large proper motions, subsequently confirmed by m…