19 بهمن 1401
محسن نژاد اصغر

محسن نژاد اصغر

مرتبه علمی: دانشیار
نشانی: گروه فیزیک دانشگاه مازندران
تحصیلات: دکترای تخصصی / فیزیک
تلفن: 09355892196
دانشکده: دانشکده علوم پایه

مشخصات پژوهش

عنوان The effect of magnetic field morphology on the structure of massive IRDC clumps
نوع پژوهش مقاله چاپ شده
کلیدواژه‌ها
ISM: structure, ISM: clouds, ISM: magnetic fields, Stars: formation, (Galaxy:) local interstellar matter
مجله ASTROPHYSICS AND SPACE SCIENCE
شناسه DOI 10.1007/s10509-018-3394-y
پژوهشگران ناهید بهمنی (نفر اول) ، محسن نژاد اصغر (نفر دوم)

چکیده

Infrared dark clouds (IRDCs) have dense elongated clumps and filaments with the favorable viewing condition of being on the near-side of a bright mid-infrared background. The clumps usually have multiple cores around the center. In this work, we study the effect of magnetic field morphology on the structure of massive IRDC clumps. To achieve this goal, we consider an axisymmetric isothermal oblate IRDC clump, embedded into a constant external magnetic field. We assume a polynomial function for the magnetic field morphology inside the clump. We use the numerical iterative methods to solve the equations: the successive over-relaxation method to find the magnetic and gravitational fluxes, and then the biconjugate gradient method to find the optimized values of mass and current densities. The results show that the IRDC clump will be very elongated along the perpendicular direction of the external magnetic field lines. Also, the assumption of choosing of a polynomial function for the magnetic field morphology leads to the formation of dense regions around the center. The greater the density of the central region, the larger the density of these dense regions and the closer to the center. The presence of these dense regions can lead to the formation of cores at these points.