activity
20082026
most citedOn the relation between the column density structures and the magnetic field orientation in the Vela C molecular complex

107 citations · 241 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.SR2026

Unveiling Dominant Toroidal Magnetic Fields in a Protostellar Outflow

Tao-Chung Ching, Zhi-Yun Li, Qizhou Zhang +6

Magnetic fields play a fundamental role in the formation of protostellar winds. In the magneto-centrifugal models, poloidal magnetic fields launch winds from accretion disks, and f…

astro-ph.GA2025

First results from ALPPS: a sub-Alfvénic streamer in SVS13A

P. C. Cortes, J. E. Pineda, T. -H. Hsieh +22

We present the first results from the ALMA Perseus Polarization Survey (ALPPS), focusing on the magnetic field in the SVS13A circumbinary disk. The dataset includes full-Stokes dus…

astro-ph.SR2025★ 2 cited

Mid-infrared extinction curve for protostellar envelopes from JWST-detected embedded jet emission: the case of TMC1A

K. D. Assani, Z. -Y. Li, J. P. Ramsey +15

Context: Dust grains are key components of the interstellar medium and play a central role in star formation, acting as catalysts for chemical reactions and as building blocks of p…

astro-ph.SR2024★ 15 cited

The Asymmetric Bipolar Fe II Jet and H2 Outflow of TMC1A Resolved with JWST's NIRSpec IFU

Korash Assani, Daniel Harsono, Jon Ramsey +10

(abridged) Protostellar outflows exhibit large variations in their structure depending on the observed gas emission. This study analyzes the atomic jet and molecular outflow in the…

astro-ph.SR2023

On the importance of disc chemistry in the formation of protoplanetary disc rings

C. A. Nolan, B. Zhao, P. Caselli +1

Radial substructures have now been observed in a wide range of protoplanetary discs (PPDs), from young to old systems, however their formation is still an area of vigorous debate.…

astro-ph.SR2020★ 21 cited

Detection of Irregular, Sub-mm Opaque Structures in the Orion Molecular Clouds: Protostars within 10000 years of formation?

Nicole Karnath, S. T. Megeath, John Tobin +10

We report ALMA and VLA continuum observations that potentially identify the four youngest protostars in the Orion Molecular Clouds taken as part of the Orion VANDAM program. These…

astro-ph.GA2017★ 107 cited

On the relation between the column density structures and the magnetic field orientation in the Vela C molecular complex

J. D. Soler, P. A. R. Ade, F. E. Angilè +27

We statistically evaluate the relative orientation between gas column density structures, inferred from Herschel submillimetre observations, and the magnetic field projected on the…

astro-ph.SR2015★ 29 cited

A high-velocity bulge RR Lyrae variable on a halo-like orbit

Andrea Kunder, R. Michael Rich, Keith Hawkins +21

We report on the RR Lyrae variable star, MACHO 176.18833.411, located toward the Galactic bulge and observed within the data from the ongoing Bulge RR Lyrae Radial Velocity Assay (…

astro-ph.SR2014★ 18 cited

Testing Magnetic Field Models for the Class 0 Protostar L1527

J. A. Davidson, Z. -Y. Li, C. L. H. Hull +10

For the Class 0 protostar, L1527, we compare 131 polarization vectors from SCUPOL/JCMT, SHARP/CSO and TADPOL/CARMA observations with the corresponding model polarization vectors of…

astro-ph.SR2010★ 17 cited

The disk-bearing young star IM Lup

H. M. Guenther, S. P. Matt, J. H. M. M. Schmitt +3

Classical T Tauri stars (CTTS) differ in their X-ray signatures from older pre-main sequence stars, e.g. weak-lined TTS (WTTS). CTTS show a soft excess and deviations from the low-…

astro-ph2008★ 32 cited

Revealing the fastest component of the DG Tau outflow through X-rays

H. M. Guenther, S. P. Matt, Z. -Y. Li

Some T Tauri stars show a peculiar X-ray spectrum that can be modelled by two components with different absorbing column densities. We seek to explain the soft X-ray component in D…