11 new active galaxy nuclei has been discovered completely in wiping the entire X -ray source conducted by researchers from the Russian Academy of Science. The Grigory USkov team has examined the X-XC X-XC sources for the Spektr-RG (SRG). To date, their studies have led to more than 50 AGN and many disaster variables. The deepest diving in physical properties and the radiological nature of these galaxies will be very important for a wide range of studies such as statistical visions, refining and testing cosmic models, classification studies, etc.
The newly found AGN classification
According to modern study, Published In astronomy messages, the newly discovered active galaxy nuclei is classified from the ARTS1-5 catalog as seyfert galaxies, seven of type 1 (SY 1), three type 1.9 (SY 1.9) and one type 2 (SY 2).
AGN or the active galaxy cores are the most brighter sources of electromagnetic radiation in the universe. These areas integrated in the middle of the galaxy are very active due to accumulation on A super black hole or stars formation activity at the Galaxy Center.
Based on its shine, AGNS is classified as seyfert and Quasars galaxies. SEYFERT galaxies are AGNS less than that as the host galaxy is clearly visible and a lot of infrared radiation is emitted, and has wide visual emissions lines.
Research results
The published paper states that 11 newly found galaxies are located relatively close, when red shifts from 0.028-0.258. X -ray is located in these sources in the range of 2 to 300 Tredecillion Erg/s, and therefore they are typical for AGNS in the current era.
One spectrum of the new AGNS, SRGA J000132.9+240237, is described by the Energy Law with a smaller slope from 0.5, indicating strong absorption and great contribution from the reflected radiation from the soil in the galaxy. The paper authors note that the longest X -ray notes are required to determine the physical properties of this AGN.
