![Observed spectra compared to laboratory data for CO (left), 13CO2 (middle), and H2O (right) ices on carbonaceous dust analogs. -- [astro-ph.GA]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/08/Molecule-specific.png?resize=1200%2C606&ssl=1)
[astro-ph.GA] Interstellar ices form on dust grains in the coldest regions of molecular clouds and preserve key volatile reservoirs that could be incorporated into protoplanetary disks during star and planet […]
astro-ph.GA
Posted inAstrochemistry
First Detection Of C2H+ In The Interstellar Medium
[astro-ph.GA] Despite the detection of nearly 350 molecules in the interstellar medium, almost half of which are carbon chains, the pathways that build molecular complexity remain poorly understood.
Posted inAstrochemistry
Photochemistry Of Interstellar Ice Forming Complex Organic Molecules
[astro-ph.GA] Astrochemistry is a well-established multidisciplinary field devoted to study molecules in space. While most astrochemists are oriented to observe molecules in the gas phase and reproduce their abundances by […]
![Herschel H2 column density map (Sadavoy et al. 2012) of Perseus starless and prestellar cores. Labeled in magenta are the locations and names of the 15 starless and prestellar cores analyzed. The star-forming regions within Perseus are denoted in black.-- [astro-ph.GA]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/08/Inventories.png?resize=1200%2C716&ssl=1)
Posted inAstrochemistry
Inventories of Rich Carbon-Chain Chemistry in Prestellar and Starless Cores in the Perseus Molecular Cloud
[astro-ph.GA] Carbon-chain molecules serve as an important reservoir of reactive organic matter that will eventually be incorporated into protoplanetary disks, planets, and cometary material. Prestellar and starless cores are composed […]
Posted inAstrochemistry
Variations in the 3.3 µm Polycyclic Aromatic Hydrocarbon Feature Across Nearby Galaxies Driven by Metallicity and Radiation Field Spectrum
[astro-ph.GA] We use JWST NIRCam imaging to investigate the 3.3 μm polycyclic aromatic hydrocarbon (PAH) feature in nearby galaxies. NIRCam observations of the 3.3 μm feature are emerging as a […]
![Simulated results with NewAthena/X-IFU (400ks exposure, binning factor 3). Figure (a) and (b) plotted the dust model against simulated data (sim. data) along the line of sight from GX 340+00 and GX 5-1, respectively. Figure (c) displays the comparison of three silicate models in GX 13+. -- [astro-ph.GA]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/08/Investigation.png?resize=1200%2C726&ssl=1)
Posted inAstrochemistry
Investigation Of Calcium Dust In The Interstellar Medium
[astro-ph.GA] Calcium is a highly depleted element in the interstellar medium (ISM), however its composition in the solid phase remains elusive. The detection of Ca-bearing dust has been limited due […]
![Three-dimensional thermal phase architecture of the local ISM. (a) Three-dimensional rendering of the cold (blue) and unstable (yellow) isosurfaces, with warm gas shown transparent. The transparent warm volume traces WNM together with unmodelled hot ionised gas, which carries negligible mass (Methods). An interactive version is available at https://sb2580.github.io/phases 3d/. (b) Slices through the Galactic plane (𝑧 = 0) of gas density 𝑛 (left), FUV radiation intensity 𝐼UV (middle), and phase classification (right). Concentric circles mark heliocentric radii of 150, 300, and 450 pc. -- [astro-ph.GA]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/07/The-first-three.png?resize=1200%2C719&ssl=1)
Posted inAstrochemistry
The First Three-dimensional Map Of Thermal Phases In The Local Interstellar Medium
[astro-ph.GA] The thermal state of interstellar gas controls whether it remains warm and diffuse or cools into dense clouds. Twentyone centimetre observations have established a statistical picture of neutral-gas phases, […]
![Sky coverage of the final sample of 1341 planet-hosting stars (yellow markers) shown in Galactic coordinates overlaid on the 2MASS near-infrared map (courtesy of ESA/Gaia/DPAC). The prominent overdensity corresponds to the Kepler mission (Borucki et al. 2010) footprint. -- [astro-ph.GA]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/07/Probing-the-origins.png?resize=1200%2C716&ssl=1)
Posted inExoplanets, -moons, -comets
Probing The Origins. III. Exoplanet Demographics Across Galactic Birth Radii
[astro-ph.GA] We quantify radial mixing in exoplanet hosts and explore links between birth environment, orbital evolution, planetary architecture, and Galactic habitability. We constructed a homogeneous catalogue by cross-matching the Encyclopaedia […]
Posted inAstrochemistry
Efficient Interstellar Grain Growth From High Sticking Coefficients On Amorphous Carbon Dust
[astro-ph.GA] Cosmic dust is the solid phase of the interstellar medium (ISM), classically assumed to be composed of carbonaceous and silicate grains with size distributions spanning ∼5 Å to ∼1 […]
![Left panel: Image of the episodic wide-angle tailed radio galaxy (RGZ J082312.9+033301) discovered by the RGZ project from Banfield et al. (2016). Right Panel: A HyMoRS from the same RGZ project displaying FR-I nature on the southern and clear edge-brightened FR-II nature on the northern side from Kapińska et al. (2017). -- [astro-ph.GA]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/07/Citizen-Science.png?resize=1200%2C719&ssl=1)
Posted inCitizen Science / Open Science
Citizen Science Research With The Square Kilometre Array Observatory (SKAO)
[astro-ph.GA] Over the past two decades, internet-enabled citizen science research (CSR) has contributed to significant discoveries while involving millions of people in the research process.