English

Possibilities of Using Middle-Band Filters to Search for Polar Candidates

Solar and Stellar Astrophysics 2020-10-28 v1 High Energy Astrophysical Phenomena Instrumentation and Methods for Astrophysics

Abstract

We present a method for searching for polar candidates using mid-band filters. One of the spectral singularities of polars is the HeIIλ4686HeII \lambda4686\AA~ strong emission line. We selected the Edmund Optics filters with central wavelengths of 470, 540, and 656 nm and a transmission bandwidth of 10 nm. These filters cover the regions of the HeIIλ4686HeII \lambda4686\AA~ line, continuum, and the HαH_\alpha line respectively. We constructed a color diagram based on the available spectra of polars and objects with a zero redshift from the SDSS archive. We show that most polars make a group with unique color indices. In practice, the method is implemented in SAO RAS at the Zeiss-1000 telescope with a new multi-mode photometer-polarimeter (MMPP). Approbation of the method with the known polars allowed us to develop two criteria to select candidates with an efficiency of up to 75\%.

Keywords

Cite

@article{arxiv.2004.11764,
  title  = {Possibilities of Using Middle-Band Filters to Search for Polar Candidates},
  author = {M. M. Gabdeev and T. A. Fatkhullin and N. V. Borisov},
  journal= {arXiv preprint arXiv:2004.11764},
  year   = {2020}
}

Comments

10 pages, 5 figures, 2 tables