3 papers
astro-ph.SR2021
The Be Star 66 Ophiuchi: 60 Years of Disk Evolution
Keegan C. Marr, Carol E. Jones, Alex C. Carciofi +5
We use a time-dependent hydrodynamic code and a non-LTE Monte Carlo code to model disk dissipation for the Be star 66 Ophiuchi. We compiled 63 years of observations from 1957 to 20…
astro-ph.GA2019
The VISCACHA survey -- deep and resolved photometry of star clusters in the Magellanic Clouds
Bruno Dias, Francisco Maia, Leandro Kerber +24
The VISCACHA (VIsible Soar photometry of star Clusters in tApii and Coxi HuguA\footnote{LMC and SMC names in the Tupi-Guarani language spoken by native people in Brazil}) Survey is…
astro-ph.SR2015
Modeling the Complete Lightcurve of omega CMa
M. R. Ghoreyshi, A. C. Carciofi, L. R. Rimulo +5
We have used the radiative transfer code HDUST to analyze and interpret the long-term photometric behavior of the Be star omega CMa, considering four complete cycles of disk format…