protostar GSS30 IRS3 Archives

Left: ALMA continuum image of GSS30 IRS3 at 1.3 mm. White contours are 5, 10, 20, 40, 60, 80, 100, 130, 160, 190, and 220 times the rms (1σ = 18.5 µJy beam´1 ). Center: Gaussian fit model image. Right: Residual from the Gaussian fit model image. White contours are -20, -10, 5, 10, 20, 40, 60, 80, 100, 130, 160, 190, and 220 times the rms. Dashed lines represent negative contours. The beam size is represented by the filled ellipse in the bottom left corner of the three images. -- astro-ph.SR

Astrogeology, Biochemistry & Organic Chemistry, Biogeochemical Cycles & Geobiology, Exoplanets, -moons, -comets, Status Report

Early Planet Formation in Embedded Disks (eDisk) XVI: An Asymmetric Dust Disk Driving a Multi-component Molecular Outflow in the Young Class 0 Protostar GSS30 IRS3

by Keith CowingAugust 11, 2024August 10, 2024

We present the results of the ALMA Large Program Early Planet Formation in Embedded disks observations of the Class 0 protostar GSS30 IRS3. Our observations included 1.3 mm continuum with […]

protostar GSS30 IRS3

Early Planet Formation in Embedded Disks (eDisk) XVI: An Asymmetric Dust Disk Driving a Multi-component Molecular Outflow in the Young Class 0 Protostar GSS30 IRS3

Relevance of the Avalon Assemblage as an Astrobiological Analog for Icy Ocean Worlds

The Climate and Potential Habitability of a Warm and Oxygenated Mars

Variable X-ray flux May Explain Variable Helium Escape From The Habitable-zone Exoplanet LHS 1140b

Spacetime Contactability in Galactic Civilization Networks: Contact Counts and Percolation

Surprisingly Enriched CO and CH4 in Halley-type Comet 13P/Olbers: Clues to Its Interstellar Heritage