Does the Magnetic Field Suppress Fragmentation in Massive Dense Cores?

نویسندگان

چکیده

Theoretical and numerical works indicate that a strong magnetic field should suppress fragmentation in dense cores. However, this has never been tested observationally relatively large sample of fragmenting massive Here we use the polarization data obtained Submillimeter Array Legacy Survey Zhang et al. to build 18 cores where both properties are studied uniform way. We measured level, Nmm, within view common all regions, 0.15 pc, with mass sensitivity about 0.5 Msun, spatial resolution 1000 au. In order obtain strength using Davis-Chandrasekhar-Fermi method, estimated dispersion position angles, velocity H13CO+(4-3) gas, density each core, averaged pc. A correlation is found between Nmm average parental although significant scatter. When large-scale systematic motions separated from only small-scale (turbulent) contribution taken into account, tentative mass-to-flux ratio, as suggested by theoretical works.

برای دانلود باید عضویت طلایی داشته باشید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

S-bearing molecules in Massive Dense Cores

Context. High-mass stars, though few in number, play a major role in the interstellar energy budget and the shaping of the Galactic environment. However, despite this importance, the formation of high-mass stars is not well understood, due to their large distances, short time scales, and heavy extinction. Aims. Chemical composition of the massive cores forming high-mass stars can put some const...

متن کامل

HNCO in massive galactic dense cores

We surveyed 81 dense molecular cores associated with regions of massive star formation and Sgr A in the JK−1K1 = 505 − 404 and 10010 − 909 lines of HNCO. Line emission was detected towards 57 objects. Selected subsamples were also observed in the 101 − 000, 404 − 303, 707 − 606, 15015 − 14014, 16016 − 15015 and 21021 − 20020 lines, covering a frequency range from 22 to 461 GHz. HNCO lines from ...

متن کامل

S-bearing molecules in massive dense cores

Context. Although few in number, high-mass stars play a major role in the interstellar energy budget and the shaping of the Galactic environment; however, the formation of high-mass stars is not well understood, because of their large distances, short time scales, and heavy extinction. Aims. The chemical composition of the massive cores forming high-mass stars can put some constraints on the ti...

متن کامل

Does a magnetic field suppress the Coulomb gap ?

We used electron-tunnelling spectroscopy to investigate the Coulomb correlation in n type Germanium. The dopant concentration was smaller than the critical concentration for the metal-insulator (Anderson) transition. The tunnelling conductance, which probes the electronic density of states, was found to depend strongly on both voltage and temperature. At low temperatures it shows a conductance ...

متن کامل

The Ionization Fraction in Dense Molecular Gas Ii: Massive Cores

We present an observational and theoretical study of the ionization fraction in several massive cores located in regions that are currently forming stellar clusters. Maps of the emission from the J = 1 → 0 transitions of CO, DCO, N2H, and HCO, as well as the J = 2 → 1 and J = 3 → 2 transitions of CS, were obtained for each core. Core densities are determined via a large velocity gradient analys...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

ژورنال

عنوان ژورنال: The Astrophysical Journal

سال: 2021

ISSN: ['2041-8213', '2041-8205']

DOI: https://doi.org/10.3847/1538-4357/abee1e