NGC 628 Archives

UVIT and JWST images of the sample of galaxies are shown in the top and bottom panels. The field of JWST observation is marked in the UVIT FUV images. The UVIT footprint with JWST observation and the corresponding JWST color composite image of the sample of galaxies are shown in the bottom panel. The JWST color composite images are generated using F770W, F1130W, and F2100W filters, which are color-coded in blue, green, and red, respectively. Blue ellipses in the UVIT footprints in the lower panel represents the PAH bright regions identified using ProFound. For all the images North is up and East to the left. -- astro-ph.GA

Astrochemistry, Astronomy & Telescopes, Imaging & Spectroscopy, Status Report

Disentangling The Association Of PAH Molecules With Star Formation : Insights From JWST And UVIT

by Keith CowingJanuary 11, 2024January 10, 2024

Polycyclic Aromatic Hydrocarbons (PAHs) are ubiquitous complex molecules in the interstellar medium and are used as an indirect indicator of star-formation.

NGC 628

Disentangling The Association Of PAH Molecules With Star Formation : Insights From JWST And UVIT

Potential Survivable Niches For Microbial Life On The Lunar South Pole

JWST Telemetry Combined With Active Coronagraphy: Raw Contrast Predictions For Exoplanet Imaging With The Habitable Worlds Observatory

Antarctica Is Home To Microbes Found Nowhere Else On Earth

Study: Peptides Can Form Well-defined Structures In Harsh, Venus-like Conditions

Modeling Carbon-Based Planets with MAGRATHEA