Interferometric Mapping of Magnetic Fields in Star‐forming Regions. I. W51 e1/e2 Molecular Cores [PDF]
S. Lai +3 more
openalex +1 more source
Polarization of starlight and thermal dust emission caused by aligned dust grains is a valuable tool to characterize magnetic fields ( B -fields) and constrain dust properties. However, the grain alignment physics is not fully understood.
Nguyen Bich Ngoc +3 more
doaj +1 more source
Star forming regions in gas-rich SO galaxies [PDF]
The first results of an H alpha imaging survey of HI rich SO galaxies, which were searched for HII regions and other sources of emission, are presented. The charge coupled device H alpha interference filter images were made of 16 galaxies. Eight of these
Eskridge, Paul B., Pogge, Richard W.
core +1 more source
[ITAL]HUBBLE SPACE TELESCOPE[/ITAL][ITAL]Hubble Space Telescope[/ITAL] Observations of Dust and Star-forming Regions in the Ocular Galaxy IC 2163 and Its Spiral Companion NGC 2207 [PDF]
D. M. Elmegreen +6 more
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Unveiling Physical Conditions and Star Formation Processes in the G47 Filamentary Cloud
We present a multiwavelength study of the filamentary cloud G47 ( d ∼ 4.44 kpc), which hosts the mid-infrared bubbles N98, B1, and B2. The SMGPS 1.3 GHz continuum map detects ionized emission toward all the bubbles, marking the first detection of ionized
O. R. Jadhav +8 more
doaj +1 more source
Nitric oxide in star-forming regions - Further evidence for interstellar N-O bonds
L. M. Ziurys +3 more
openalex +1 more source
The Alignment of the Magnetic Field and Collimated Outflows in Star‐forming Regions: The Case of NGC 2071 [PDF]
Martin Houde +4 more
openalex +1 more source
Structure of photodissociation fronts in star-forming regions revealed by observations of high-J CO emission lines with Herschel. [PDF]
Joblin C +19 more
europepmc +1 more source
Quantification of the Age Dependence of Mid-infrared Star Formation Rate Indicators
We combine James Webb Space Telescope images of the nearby galaxy NGC 5194 in the hydrogen recombination line Pa α (1.8756 μ m) from the Cycle 1 program JWST-FEAST with 21 μ m dust continuum images from the Cycle 2 Treasury program JWGT to quantify the ...
Daniela Calzetti +35 more
doaj +1 more source

