KONSENTRATSIYA PARAMETRI VA SHARSIMON TO‘DALARDAGI ORALIQ MASSALI QORA O‘RALAR ORASIDAGI BOG‘LANISH
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Ushbu maqolada sharsimon to‘dalar (ShT) markaziga tomon yulduzlar zichligining ortish tezligini xarakterlovchi kontsentratsiya parametri va markaziy oraliq massali qora o‘ralar (OMQO’) massalari o‘rtasidagi empirik bog‘liqlik o‘rganiladi. Tadqiqotda faqat nazariy usullar yordamida hisoblangan OMQO’ massalari ko‘rib chiqiladi. Kontsentratsiya parametr qiymatlari Gaia DR2 kuzatuvlari asosida olingan sirt zichligi profillari bo‘yicha hisoblab chiqilgan. Kontsentratsiya parametri markaziy OMQO’larning xususiyatlari va shakllanish jarayonlarini baholashda diagnostik vosita sifatida qo‘llanishi mumkin.
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