activity
19932020
most citedDetection of Gamma-ray Emission from the Eta-Carinae Region

114 citations · 238 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.SR2020★ 5 cited

Asymmetrical nebula of the M33 variable GR290 (WR/LBV)

Olga V. Maryeva, Gloria Koenigsberger, Sergey V. Karpov +5

Context: GR290 (M33 V0532=Romano's star) is a luminous M33 object undergoing photometric variability typical for luminous blue variable (LBV) stars. It lies inside Wolf-Rayet regio…

astro-ph.SR2019★ 7 cited

The History Goes On: Century Long Study of Romano's Star

Olga Maryeva, Roberto F. Viotti, Gloria Koenigsberger +3

GR 290 (M 33 V0532 = Romano's Star) is a unique variable star in the M33 galaxy, which simultaneously displays variability typical for luminous blue variable (LBV) stars and physic…

astro-ph.SR2018★ 7 cited

Wind and nebula of the M33 variable GR290 (WR/LBV)

Olga Maryeva, Gloria Koenigsberger, Oleg Egorov +4

Context: GR290 (M33/V532=Romano's Star) is a suspected post-LBV star located in M33 galaxy that shows a rare Wolf-Rayet spectrum during its minimum light phase. In spite of many st…

astro-ph.SR2016★ 11 cited

GR 290 (Romano's Star): 2. Light history and evolutionary state

V. F. Polcaro, O. Maryeva, R. Nesci +11

We have built the historical light curve of the luminous variable GR 290 back to 1901, from old observations of the star found in several archival plates of M 33. These old recordi…

astro-ph.SR2010

The Extreme LBV Star GR290 (Romano's Star) in M33. Optical Spectrophotometric Monitoring

V. F. Polcaro, R. F. Viotti, C. Rossi +3

We study the long term, S Dor-type variability and the present hot phase of the LBV star GR290 (Romano's Star) in M33 in order to investigate possible links between the LBV and WNL…

astro-ph.HE2009★ 25 cited

The origin of the supersoft X-ray--optical/UV flux anticorrelation in the symbiotic binary AG Draconis

A. Skopal, M. Sekeras, R. Gonzalez-Riestra +1

AG Draconis produces a strong supersoft X-ray emission.The X-ray and optical/UV fluxes are in a strict anticorrelation throughout the active and quiescent phases. The aim of this c…