1403/01/09
محسن نژاد اصغر

محسن نژاد اصغر

مرتبه علمی: دانشیار
ارکید:
تحصیلات: دکترای تخصصی
اسکاپوس:
دانشکده: دانشکده علوم پایه
نشانی:
تلفن: 09355892196

مشخصات پژوهش

عنوان
The effect of magnetic field morphology on the structure of massive IRDC clumps
نوع پژوهش
JournalPaper
کلیدواژه‌ها
ISM: structure, ISM: clouds, ISM: magnetic fields, Stars: formation, (Galaxy:) local interstellar matter
سال
2018
مجله ASTROPHYSICS AND SPACE SCIENCE
شناسه DOI
پژوهشگران Nahid Bahmani ، Mohsen Nejad-Asghar

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.