papers

Publications (7)

astro-ph2002

Discovery of New Milky Way Star Clusters Candidates in the 2MASS Point Source Catalog

V. D. Ivanov, J. Borissova, P. Pessev +2

A systematic search of the 2MASS point source catalog, covering 47% of the sky, was carried out aiming to reveal any hidden globular clusters in our Galaxy. Eight new star clusters…

astro-ph2003

Discovery of New Milky Way Star Cluster Candidates in the 2MASS Point Source Catalog II. Physical Properties of the Star Cluster CC01

J. Borissova, P. Pessev, V. D. Ivanov +3

Three new obscured Milky Way clusters were detected as surface density peaks in the 2MASS point source catalog during our on-going search for hidden globular clusters and massive A…

astro-ph2005

Discovery of new Milky Way star cluster candidates in the 2MASS Point Source Catalog IV. Follow-up observations of cluster candidates in the Galactic plane

V. D. Ivanov, J. Borissova, F. Bresolin +1

Nearly 500 cluster candidates have been reported by searches based on the new all-sky near infrared surveys. The true nature of the majority of these objects is still unknown. This…

astro-ph.GA2016

Nuevos resultados sobre la cinemática global y nuclear de NGC 253: movimientos no circulares y emisión en Br-gamma

J. A. Camperi, G. I. Gunthardt, R. J. Diaz +3

Continuing with previous research (Camperi et al. 2011),new heliocentric radial velocity distributions are presented for the nearby galaxy NGC 253, obtained from the ionized hydrog…

astro-ph.SR2013

Haffner 16: A Young Moving Group in the Making

T. J. Davidge, E. R. Carrasco, C. Winge +4

The photometric properties of main sequence (MS) and pre-main sequence (PMS) stars in the young cluster Haffner 16 are examined using images recorded with the Gemini South Adaptive…

astro-ph.SR2020

AT 2019abn: multi-wavelength observations over the first 200 days

S. C. Williams, D. Jones, P. Pessev +8

AT 2019abn was discovered in the nearby M51 galaxy by the Zwicky Transient Facility at more than two magnitudes and around three weeks prior to its optical peak. We aim to conduct…