collaborators

5 papers

astro-ph.GA2026

Formation of Isotopically Heterogeneous Molecular Cloud Cores in Filamentary Molecular Clouds

Yoshiaki Misugi, Shu-ichiro Inutsuka, Taishi Nakamoto +1

Meteorite analysis shows that the older solids of the solar system, such as the calcium-aluminum-rich inclusions (CAIs), have isotopic inhomogeneity. This indicates that the isotop…

astro-ph.GA2026

Probing the ion-neutral drift velocity towards the L1544 prestellar core: Detection of ambipolar diffusion using ND and para-NHD

Doris Arzoumanian, Silvia Spezzano, Tommaso Grassi +9

The dynamical role of the magnetic field in the star formation process is tightly linked to the coupling between matter and the field. This coupling is due to the interaction betwe…

astro-ph.GA2026

A differentiable and optimizable 3D model for interpretation of observed spectral data cubes

T. Grassi, J. E. Pineda, S. Spezzano +6

Molecular spectral cubes of prestellar cores encode the information on the physical and chemical properties of these objects along the line of sight. To retrieve this information,…

astro-ph.GA2026

Ion-Neutral Drift Velocity as a Diagnostic of Dust Growth and Magnetic Field in Star-Forming Environments

Haruka Fukihara, Yusuke Tsukamoto, Hiroyuki Hirashita +2

Recent observations have revealed that the ion-neutral drift velocity in star-forming molecular clouds and dense cores is on the order of 100 m s^-1. Theoretical studies have shown…

astro-ph.GA2025

Fragmenting Filaments and Evolving Cores -- Insights from Dust Polarisation Study of a filament in Northern Orion B

Kshitiz K. Mallick, Doris Arzoumanian, Satoko Takahashi +5

We present an analysis of polarised dust emission at 850 micron for a parsec long filament in the northern part of the Orion B molecular cloud. The region was observed by the JCMT…