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20192026
most citedAn Origin for the Angular Momentum of Molecular Cloud Cores: a Prediction from Filament Fragmentation

28 citations · 68 across the 11 of their papers we have counts for

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Showing 2026Show all

8 papers · 1 filter

astro-ph.GA2026

B-fields In STar-forming Region Observations (BISTRO): Dual-Wavelength Constraints on Size-Dependent Grain Alignment in Star-Forming Regions

Ray S. Furuya, David Berry, Pierre Bastien +65

We compared 450 and 850 m POL-2 observations from the James Clerk Maxwell Telescope at resolution. The median absolute difference in polarization angle between bands is…

astro-ph.GA2026

B-fields In STar-forming Region Observations (BISTRO): Technical Foundations for Quantitative 450/850 m JCMT SCUBA-2/POL-2 Polarimetry

Ray S. Furuya, David Berry, Pierre Bastien +59

We present five technical validations of SCUBA-2/POL-2 polarimetry on the James Clerk Maxwell Telescope at 450 and 850 m, using 174 archival fields in 69 molecular cloud regions…

astro-ph.GA2026

Dust Growth in Evolving Filamentary Molecular Clouds: Signatures in Ionization, Resistivity, and Infrared Scattering

Hayato Uchimura, Yoshiaki Misugi, Daisuke Takaishi +4

Studies of dust growth in molecular clouds often prescribe the collapse history, leaving unclear how magnetic regulation of core formation shapes dust evolution and its observable…

astro-ph.GA2026

Corona Australis 151: an extremely young protostar

E. Redaelli, S. Spezzano, P. Caselli +9

Context. Prestellar cores are the birthplace of stars and planetary systems, but they are short-lived objects, since the initial stages of dense core evolution, collapse, and the f…

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★ 1 cited

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…