V2282 Sgr Revisited
DOI:
https://doi.org/10.14311/APP.2014.01.0118Abstract
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.Downloads
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Published
2014-12-04
How to Cite
Nesci, R., Rossi, C., Frasca, A., Marilli, E., Persi, P., & Cornero, N. (2014). V2282 Sgr Revisited. Acta Polytechnica CTU Proceedings, 1(1), 118–122. https://doi.org/10.14311/APP.2014.01.0118
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