activity
20042020
most citedSpiral structure of the Third Galactic Quadrant and the solution to the Canis Major debate

97 citations · 184 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2020

Embedded clusters: upgrading visual and infrared photometric analysis with Gaia DR2 and ASteCA

E. E. Giorgi, G. R. Solivella, A. Cruzado +3

Embedded clusters are groups of stars which have not dispersed yet the residual of the parental cloud where they were born so getting precise distances and properties of these grou…

astro-ph.GA2020★ 21 cited

Sixteen overlooked open clusters in the fourth Galactic quadrant. A combined analysis of UBVI photometry and Gaia DR2 with ASteCA

G. I. Perren, E. E. Giorgi, A. Moitinho +3

Aims: This paper has two main objectives: (1) To determine the intrinsic properties of 16 faint and mostly unstudied open clusters in the poorly known sector of the Galaxy at 270$^…

astro-ph.GA2015★ 6 cited

The nearby Galaxy structure toward the Vela Gum nebula

E. E. Giorgi, G. R. Solivella, G. I. Perren +1

We report on photometry and spectroscopy for MK classification purposes carried out in the fields of five open clusters projected against the Vela Gum in the Third Galactic…

astro-ph.GA2014★ 23 cited

The thickening of the thin disk in the third Galactic quadrant

Giovanni Carraro, Ruben A. Vazquez, Edgardo Costa +2

In the third Galactic quadrant (180 < l < 270) of the Milky Way, the Galactic thin disk exhibits a significant warp ---shown both by gas and young stars--- bending down a few kpc b…

astro-ph.SR2014★ 7 cited

On the Crucial Cluster Andrews-Lindsay 1 and a 4% Distance Solution for its PN

D. Majaess, G. Carraro, C. Moni Bidin +5

Andrews-Lindsay 1 is a pertinent open cluster granted it may host the planetary nebula PHR 1315-6555, yet ambiguities linger concerning its fundamental parameters (>50% scatter). N…

astro-ph.SR2014★ 8 cited

NGC 4337: an over-looked old cluster in the inner disc of the Milky Way

Giovanni Carraro, Edgard Giorgi, Edgardo Costa +1

Galactic open clusters do not survive long in the high density regions of the inner Galactic disc. Inside the solar ring only 11 open clusters are known with ages older than one Gy…