activity
19962021
most citedThe extent of NGC 6822 revealed by its C stars population

99 citations · 555 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.SR2021

Hot Degenerates in the MCT Survey. III. A Sample of White Dwarf Stars in the Southern Hemisphere

P. Bergeron, F. Wesemael, G. Fontaine +7

We present optical spectra of 144 white dwarfs detected in the Montreal-Cambridge-Tololo (MCT) colorimetric survey, including 120 DA, 12 DB, 4 DO, 1 DQ, and 7 DC stars. We also per…

astro-ph.SR2012★ 29 cited

Extension of the C star rotation curve of the Milky Way to 24 kpc

P. Battinelli, S. Demers, C. Rossi +1

Demers and Battinelli published, in 2007 the rotation curve of the Milky Way based on the radial velocity of carbon stars outside the Solar circle. Since then we have established a…

astro-ph2007★ 23 cited

The assessment of the near infrared identification of Carbon stars. I. The Local Group galaxies WLM, IC 10 and NGC 6822

P. Battinelli, S. Demers, F. Mannucci

{The selection of AGB C and M stars from NIR colours has been done in recent years using adjustable criteria that are in needs of standardization if one wants to compare, in a cohe…

astro-ph2007★ 16 cited

The size and structure of the spheroid of IC 1613

P. Battinelli, S. Demers, É. Artigau

Nearby galaxies, spirals as well as irregulars, have been found to be much larger than previously believed. The structure of the huge spheroid surrounding dwarf galaxies could give…

astro-ph2006★ 26 cited

C stars in the outer spheroid of NGC 6822

S. Demers, P. Battinelli, E. Artigau

From a 2 x 2 degree survey of NGC 6822 we have previously established that this Local Group dwarf irregular galaxy possesses a huge spheroid having more than one degree in length.…

astro-ph2006★ 44 cited

Photometric Survey of the Polar ring galaxy NGC 6822

P. Battinelli, S. Demers, W. E. Kunkel

We have previously established, from a carbon star survey, that the Local Group dwarf irregular galaxy NGC 6822 is much larger than its central bright core. Four MegaCam fields are…