@InProceedings{SouzaOlivRodrLima:2021:SpAnMC,
               author = "Souza, D. C. and Oliveira, A. S. and Rodrigues, Cl{\'a}udia 
                         Vilega and Lima, Isabel de Jesus",
          affiliation = "{Universidade do Vale do Para{\'{\i}}ba (UNIVAP)} and 
                         {Universidade do Vale do Para{\'{\i}}ba (UNIVAP)} and {Instituto 
                         Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de 
                         Pesquisas Espaciais (INPE)}",
                title = "Spectroscopic analysis of the mCV candidate CSS0357+10 with SOAR 
                         Telescope data",
                 year = "2021",
         organization = "Simp{\'o}sio Brasileiro de Geof{\'{\i}}sica Espacial e 
                         Aeronomia, 8. (SBGEA)",
             abstract = "Cataclysmic variables are binary systems where the primary 
                         component is a white dwarf star and the secondary is a main 
                         sequence star, usually a red dwarf. Due to the proximity of the 
                         system components the secondary star fills its Roche lobe causing 
                         a flow of ionized gas expelled by the internal Lagrange point 
                         forming an accretion disk around the primary. Some of these white 
                         dwarfs may have a magnetic field strong enough to change the path 
                         of the gas causing it to follow the lines of its field to form an 
                         accretion column that collides with the white dwarf near its 
                         magnetic pole instead of form a disc. In others the disk is 
                         partially formed with its internal part following the magnetic 
                         field. The first is known as polar and the second as intermediate 
                         polar (IPs), both are types of magnetic cataclysmic variables 
                         (mCVs). In our project to search and characterize new mCVs several 
                         candidates are selected from the Catalina Real Time Transient 
                         photometric survey (CRTS) to confirm whether the system belongs to 
                         this class. Several systems have already been confirmed as mCV. 
                         Among them CSS 0357+10 which had also been identified as an x-ray 
                         source was chosen for a more detailed study. In this work the 
                         analysis of the spectrum of this system obtained in the SOAR 
                         telescope was performed. The spectrum is dominated by hydrogen 
                         emission lines in the Balmer series and He II ionization 
                         characteristic, properties of a mCV spectrum.",
  conference-location = "Online",
      conference-year = "22-26 mar.",
             language = "en",
        urlaccessdate = "09 maio 2024"
}