dust clouds Archives

CO brightness temperature maps for Cloud 378 at various vLSR. The black, cyan, and yellow polygons denote CO emission significance at 3σ, 6σ, and 9σ, respectively. The lines in the color bar indicate the CO emission at different levels. The red polygon highlights the dust contour boundary of the cloud as identified by Chen et al. (2020b). The method for calculating the dust contour threshold, Amin V , is described in Section 2.1. -- astro-ph.GA

Astrochemistry, Astrogeology, Biochemistry & Organic Chemistry, Interstellar, Status Report

The Correlation Between Dust and Gas Contents in Molecular Clouds

by Keith CowingSeptember 16, 2024September 16, 2024

Molecular clouds are regions of dense gas and dust in space where new stars and planets are born. There is a strong correlation between the distribution of dust and molecular […]

dust clouds

The Correlation Between Dust and Gas Contents in Molecular Clouds

A Martian Horizon Last Monday Afternoon

Habitable-zone Earths At The Detection Frontier: Measured Completeness And False-alarm Rate Of A Transit Pipeline For The PLATO M-dwarf Sample

A Homogeneous Survey Of JWST MIRI Transmission Spectra Of 10 Exoplanets

Retrieving Ocean Glint Reflectance Signatures From Directly Imaged Earth-like Exoplanets

Analytical Platform (Microsampling, Catapulting, Trapping, and LIBS) for the Characterization of Discrete Domains in Samples of Astrochemical Interest