[PDF] Top 20 Magnetic fields at the onset of high-mass star formation

... various magnetic field vectors, and integration of multiple com- ponents along the line may decrease the measurable polarization angle compared to the true dispersion of the magnetic field ...the ... See full document

... the formation of high-mass stars and their low-mass counterparts, intermediate-mass (IM) stars are of interest as they provide a bridge between the two mass ...the ... See full document

... magnetized star formation in two main ways beyond the studies mentioned ...the magnetic fields which did not allow magnetic fields to be wound ... See full document

... the star is plotted as a function of the energy density ...maximum mass allowable for a given star, and it is therefore connected with astrophysical ...average mass is ≈ ... See full document

... Star formation simulations of a strongly magnetic medium with turbulent initial conditions (Nakamura & Li, 2005; Basu et ...of magnetic fields aligned perpendicular to the filaments ... See full document

... along magnetic field lines anchored in the circumstellar disk, are directed close to its rotation axis, along its angular momentum vector, and orthogonal to any attendant accretion disk, respectively (Pudritz ... See full document

... of star formation that include strong magnetic fields under the ideal MHD approximation fail to form discs during the star forming process; this is known as the magnetic braking ... See full document

... of star formation and evolution, and the cycle of insterstellar material, including dust grains and ...example, magnetic fields have been found to play a role in circumstellar disks and jets ... See full document

... the formation of magnetic spots. In principle the magnetic field evolution is coupled to its thermal evolution, as conductivity is a func- tion of temperature (Chugunov ...the magnetic field ... See full document

... the formation and growing of the fila- ments (see also Heitsch ...the magnetic field lines. As a result of the mass collection along preferred directions, velocity gradients perpendicular to the ... See full document

... of star formation and AGN to the bolometric emission from ...and star formation make impor- tant contributions, was not completely covered with good sen- sitivity by Spitzer or by ground-based ... See full document

... exciting star(s) of VLA 1 is not seen in either the 2MASS or Gemini North near-IR ...single star, the zero-age main sequence (ZAMS) luminosities given in Panagia (1973) and a distance of 1 kpc, the spectral ... See full document

... the magnetic field strength used was ...the magnetic properties of these magnetic nanoparticles in large magnetic field strength and to identify its magnetic and motion dynamics in ... See full document

... of magnetic field lines and “chopping” the reconnection layer into smaller ...the formation of “plasma islands” in the reconnection region, a piling-up of these islands around the reconnection layer could ... See full document

... Two glaring and intriguing problems remain to be solved in this field: the origin of the supersonic turbulence observed throughout a molecular cloud, and the driving mechanism of the pow[r] ... See full document

... mass star formation region ( HMSFR ) known, with only the Orion Nebula being ...generate high-mass ...individual high-mass ...and high angular resolution images of ... See full document

... non-linear high dimensional data (Koho- nen, ...spectra, star/galaxy classifications, gamma-ray burst clustering and light curve classification) and photometric redshift estimation ... See full document

... colour mass relation of all galaxies in the matched ...are formation from NUV (hereafter (NUV − r) blue fraction), using our definitions from ...residual star formation threshold, which is ... See full document

... Figure 2 shows the typical results of the temperature dependence of the magnetization (M-T curves) of MnBi in various magnetic fields up to 10 T. Here, the data were taken in heating process. In this figure, the ... See full document

... exceptionally high mass without ev- idence of clusters merits ...Wolf–Rayet star (see ...The star displays excess emission in the mid-IR although the cause is still unclear, however the ... See full document