V2282 Sgr Revisited
| dc.contributor.author | Nesci, Roberto | |
| dc.contributor.author | Rossi, Corinne | |
| dc.contributor.author | Frasca, Antonio | |
| dc.contributor.author | Marilli, Ettore | |
| dc.contributor.author | Persi, Paolo | |
| dc.contributor.author | Cornero, Nicola | |
| dc.date.accessioned | 2023-01-18T14:10:39Z | |
| dc.date.available | 2023-01-18T14:10:39Z | |
| dc.date.issued | 2014 | |
| dc.identifier.citation | Acta Polytechnica. 2014, vol. 1, no. 1, p. 118-122. | |
| dc.identifier.issn | 1210-2709 (print) | |
| dc.identifier.issn | 1805-2363 (online) | |
| dc.identifier.uri | http://hdl.handle.net/10467/105701 | |
| dc.description.abstract | 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. | en |
| dc.format.mimetype | application/pdf | |
| dc.language.iso | eng | |
| dc.publisher | České vysoké učení technické v Praze | cs |
| dc.publisher | Czech Technical University in Prague | en |
| dc.relation.ispartofseries | Acta Polytechnica | |
| dc.relation.uri | https://ojs.cvut.cz/ojs/index.php/APP/article/view/2360 | |
| dc.rights | Creative Commons Attribution 4.0 International License | en |
| dc.rights.uri | http://creativecommons.org/licenses/by/4.0/ | |
| dc.title | V2282 Sgr Revisited | |
| dc.type | article | en |
| dc.date.updated | 2023-01-18T14:10:39Z | |
| dc.identifier.doi | 10.14311/APP.2014.01.0118 | |
| dc.rights.access | openAccess | |
| dc.type.status | Peer-reviewed | |
| dc.type.version | publishedVersion |
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