We present spatially resolved Keck/NIRC2 images of a stellar occultation by Titan on September 5, 2022 and compare them to predictions from concurrent ALMA observations and a suite of General […]
ALMA
A Deep Search For Ethylene Glycol And Glycolonitrile In The V883 Ori Protoplanetary Disk
Ethylene glycol ((CH2OH)2, hereafter EG) and Glycolonitrile (HOCH2CN, hereafter GN) are considered molecular precursors of nucleic acids.
First Detection Of Ethylene Oxide And Acetaldehyde In Hot Core G358.93−0.03 MM1: Tracing Prebiotic Oxygen Chemistry
Ethylene oxide (c-C2H4O) and its isomer, acetaldehyde (CH3CHO), are important complex organic molecules owing to their potential role in the formation of amino acids (R-CH(NH2)-COOH) in ISM.
Formation Of Exoplanet AB Aurigae b Detected in H-alpha Light
Small rocky planets like Earth, which can harbor life, and giant gas planets like Jupiter are born around stars like the Sun. Their birthplace is a thin, disk-shaped structure of […]
Fomalhaut’s Warped Ring Is Shaped By Evolving Planets
Astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA) have made the highest resolution image to date, revealing new insights into the unusual and mysterious architecture of the debris disk encircling […]
Butterfly Nebula (NGC 6302) Reveals Clues To Earth’s Creation
Clues about how worlds like Earth may have formed have been found buried at the heart of a spectacular ‘cosmic butterfly’.
Warped Protoplanetary Discs Reshape Ideas About How Planets Form
The textbook picture of how planets form – serene, flat discs of cosmic dust – has just received a significant cosmic twist. New research, published in the Astrophysical Journal Letters, […]
Cosmic Cascades: How Disk Substructure Regulates The Flow Of Water To Inner Planetary Systems
The influx of icy pebbles to the inner regions of protoplanetary disks constitutes a fundamental ingredient in most planet formation theories.
Linking Planet Formation To Exoplanet Characteristics: C/O As A Diagnostic Of Planet Formation
Gas-giant exoplanets are test cases for theories of planet formation as their atmospheres are proposed to carry signatures of their formation within the protoplanetary disk.
MINDS. Young Binary Systems With JWST/MIRI: Variable Water-rich Primaries And Extended Emission
As part of the JWST GTO program MINDS, we analyze the mid-infrared emission of three Class II binary systems: VW Cha, WX Cha, and RW Aur, to investigate the impact […]
