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Interferometric observations of magnetic fields in forming stars
CLH Hull, Q Zhang - Frontiers in Astronomy and Space Sciences, 2019 - frontiersin.org
The magnetic field is a key ingredient in the recipe of star formation. However, the
importance of the magnetic field in the early stages of the formation of low-and high-mass …
importance of the magnetic field in the early stages of the formation of low-and high-mass …
Zooming in on individual star formation: low-and high-mass stars
Star formation is a multi-scale, multi-physics problem ranging from the size scale of
molecular clouds (∼ 10 ∼10 s pc) down to the size scales of dense prestellar cores (∼ 0.1 …
molecular clouds (∼ 10 ∼10 s pc) down to the size scales of dense prestellar cores (∼ 0.1 …
Magnetic fields in star formation: from clouds to cores
In this chapter we review recent advances in understanding the roles that magnetic fields
play throughout the star formation process, gained through observations and simulations of …
play throughout the star formation process, gained through observations and simulations of …
PDRs4All: A JWST early release science program on radiative feedback from massive stars
The James Webb Space Telescope (JWST, Gardner et al. 2006) is a 6.5 m space telescope
launched in 2021 December and is developed by the National Aeronautics and Space …
launched in 2021 December and is developed by the National Aeronautics and Space …
PDRs4All-II. JWST's NIR and MIR imaging view of the Orion Nebula
Context. The James Webb Space Telescope (JWST) has captured the most detailed and
sharpest infrared (IR) images ever taken of the inner region of the Orion Nebula, the nearest …
sharpest infrared (IR) images ever taken of the inner region of the Orion Nebula, the nearest …
PICO: Probe of inflation and cosmic origins
The Probe of Inflation and Cosmic Origins (PICO) is an imaging polarimeter that will scan the
sky for 5 years in 21 frequency bands spread between 21 and 799 GHz. It will produce full …
sky for 5 years in 21 frequency bands spread between 21 and 799 GHz. It will produce full …
Expanding bubbles in Orion A:[C ii] observations of M 42, M 43, and NGC 1977
CHM Pabst, JR Goicoechea, D Teyssier… - Astronomy & …, 2020 - aanda.org
Context. The Orion Molecular Cloud is the nearest massive-star forming region. Massive
stars have profound effects on their environment due to their strong radiation fields and …
stars have profound effects on their environment due to their strong radiation fields and …
High-accuracy estimation of magnetic field strength in the interstellar medium from dust polarization
Context. A large-scale magnetic field permeates our Galaxy and is involved in a variety of
astrophysical processes, such as star formation and cosmic ray propagation. Dust …
astrophysical processes, such as star formation and cosmic ray propagation. Dust …
Using Herschel and Planck observations to delineate the role of magnetic fields in molecular cloud structure
JD Soler - Astronomy & Astrophysics, 2019 - aanda.org
We present a study of the relative orientation between the magnetic field projected onto the
plane of sky (B⊥) on scales down to 0.4 pc, inferred from the polarized thermal emission of …
plane of sky (B⊥) on scales down to 0.4 pc, inferred from the polarized thermal emission of …
The role of magnetic fields in protostellar outflows and star formation
RE Pudritz, TP Ray - Frontiers in Astronomy and Space Sciences, 2019 - frontiersin.org
The role of outflows in the formation of stars and the protostellar disks that generate them is
a central question in astrophysics. Outflows are associated with star formation across the …
a central question in astrophysics. Outflows are associated with star formation across the …