activity
20242026
most citedSIMPLIFI -- Study of Interstellar Magnetic Polarization: a Legacy Investigation of Filaments. I. Magnetically-Guided Accretion onto the DR21 Ridge

1 citations · 1 across the 2 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2026

Using Scattered Near-Infrared Light to Map Water Ice in Prestellar Cores with SPHEREx

Tamojeet Roychowdhury, Jennifer B. Bergner, Jens Kauffmann +2

We present the first coreshine-derived, spatially-resolved maps of the 3 m HO ice absorption feature in four prestellar cores, using SPHEREx spectra. Ices are a key compone…

astro-ph.GA20261 cited

SIMPLIFI -- Study of Interstellar Magnetic Polarization: a Legacy Investigation of Filaments. I. Magnetically-Guided Accretion onto the DR21 Ridge

Thushara G. S. Pillai, Jens Kauffmann, Juan D. Soler +15

We present first results from SIMPLIFI (Study of Interstellar Magnetic Polarization: a Legacy Investigation of Filaments), a SOFIA/HAWC+ polarimetric survey of Galac…

astro-ph.GA2025

Grain alignment and dust evolution physics with polarisation (GRADE-POL). I. Dust polarisation modelling for isolated starless cores

Le Ngoc Tram, Thiem Hoang, Alex Lazarian +6

The polarisation of light induced by aligned interstellar dust serves as a significant tool in investigating cosmic magnetic fields, dust properties, and poses a challenge in chara…

astro-ph.GA2025

FIELDMAPS Data Release: Far-Infrared Polarization in the "Bones" of the Milky Way

Simon Coudé, Ian W. Stephens, Philip C. Myers +13

Polarization observations of the Milky Way and many other spiral galaxies have found a close correspondence between the orientation of spiral arms and magnetic field lines on scale…

astro-ph.GA2025

Magnetic Fields in the Bones of the Milky Way

Ian W. Stephens, Simon Coude, Philip C. Myers +20

Stars primarily form in galactic spiral arms within dense, filamentary molecular clouds. The largest and most elongated of these molecular clouds are referred to as ``bones," which…

astro-ph.GA2024

Revisiting rotationally excited CH at radio wavelengths: A case study towards W51

Arshia M. Jacob, Meera Nandakumar, Nirupam Roy +7

Ever since they were first detected in the interstellar medium, the radio wavelength (3.3 GHz) hyperfine-structure splitting transitions in the rotational ground state of CH have b…