@article {28422,
	title = {The absolute parameters of the detached eclipsing binary V482 Per},
	volume = {41},
	year = {2015},
	month = {2015/11/1},
	pages = {42 - 47},
	abstract = {We present the results of a spectroscopic, photometric and orbital period variation analysis of the detached eclipsing binary V482 Per. We derived the absolute parameters of the system (M<SUB>1</SUB> = 1.51 M<SUB>⊙</SUB>, M<SUB>2</SUB> = 1.29 M<SUB>⊙</SUB>, R<SUB>1</SUB> = 2.39 R<SUB>⊙</SUB>, R<SUB>2</SUB> = 1.45 R<SUB>⊙</SUB>, L<SUB>1</SUB> = 10.15 L<SUB>⊙</SUB>, L<SUB>2</SUB> = 3.01 L<SUB>⊙</SUB>) for the first time in literature, based on an analysis of our own photometric and spectroscopic observations. We confirm the nature of the variations observed in the system{\textquoteright}s orbital period, suggested to be periodic by earlier works. A light time effect due to a physically bound, star-sized companion (M<SUB>3</SUB> = 2.14 M<SUB>⊙</SUB>) on a highly eccentric (e = 0.83) orbit, seems to be the most likely cause. We argue that the companion can not be a single star but another binary instead. We calculated the evolutionary states of the system{\textquoteright}s components, and we found that the primary is slightly evolving after the main sequence, while the less massive secondary lies well inside it.},
	keywords = {Astrophysics - Solar and Stellar Astrophysics, Stars: binaries: eclipsing, stars: fundamental parameters, Stars: individual (V482 Per), Stars: individual (V482~Per)},
	isbn = {1384-1076},
	url = {https://ui.adsabs.harvard.edu/abs/2015NewA...41...42B},
	author = {Ba{\c s}t{\"u}rk, {\"O}. and Zola, S. and Liakos, A. and Nelson, R. H. and Gazeas, K. and {\"O}zavc{\i}, {\.I}. and Y{\i}lmaz, M. and {\c S}enavc{\i}, H. V. and Zakrzewski, B.}
}
