V2282 Sgr Revisited


  • Roberto Nesci INAF-IASF, via Fosso del Cavaliere 100, 00133 Roma, Italy
  • Corinne Rossi University La Sapienza, P.le A. Moro 2, 00186 Roma, Italy
  • Antonio Frasca INAF/OACt, Catania, Italy
  • Ettore Marilli INAF/OACt, Catania, Italy
  • Paolo Persi INAF-IASF, via Fosso del Cavaliere 100, 00133 Roma, Italy
  • Nicola Cornero CDSO, Aosta, Italy




The nature of V2282 Sgr is examined on the basis of several multiband observations: a 20 years long I-band light curve of V2282 Sgr obtained from archive photographic plates of the Asiago and Catania Observatories; a CCD R-band light curve obtained at Cornero Observatory; JHK photometry from 2MASS and UKDISS; Spitzer IRAC and MIPS images; optical spectra from Loiano Observatory; X-ray flux from CHANDRA. The star has a K-type spectrum with strong emission lines and is irregularly variable at all wavebands. The overall evidences suggest that V2282 Sgr is a Pre Main Sequence star with an accretion disk.


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How to Cite

V2282 Sgr Revisited. (2014). Acta Polytechnica CTU Proceedings, 1(1), 118-122. https://doi.org/10.14311/APP.2014.01.0118