Category: astro-ph - Keerthi Vasan GC

What’s the storyline?: may 05, 2022

cosmicnoon_r6mdvbMay 9, 2022

Study of the hot intracluster medium
- Plasma physics of the intracluster medium

The morphology of the cold molecular clouds and
- The SEDIGISM survey: Molecular cloud morphology. II. Integrated source properties

The deep gravitational potential that holds them all together
- Deep Potential: Recovering the gravitational potential from a snapshot of phase space

What’s the storyline? :april20,2022

cosmicnoon_r6mdvbApril 26, 2022

Relationship between the information content in life and the information content in the Universe:
- Biocosmology: Towards the birth of a new science

Finding civilizations with Dyson spheres:
- Infrared and Optical Detectability of Dyson Spheres at White Dwarf Stars

Local habitable environments (our sun and Proxima Centauri) :
- Detection of stellar-like abundance anomalies in the slow solar wind
- The high energy spectrum of Proxima Centauri simultaneously observed at X-ray and FUV wavelengths

Exploring the Milky Way’s family tree:
- A new member of the Milky Way’s family tree: Characterizing the Pontus merger of our Galaxy

A photon from the FUV background knocks you out. Uh oh!
- The Far Ultraviolet Background

astro-ph astronomy astroph

What’s the storyline? :april21,2022

cosmicnoon_r6mdvbApril 24, 2022

James webb and blackholes:
- The Age of Discovery with the James Webb: Excavating the Spectral Signatures of the First Massive Black Holes

Blackholes and supersonic turbulence :
- Signature of Supersonic Turbulence in Galaxy Clusters Revealed by AGN-driven Hα Filaments

Feedback and Massive stars:
- A Massive Star is Born: How Feedback from Stellar Winds, Radiation Pressure, and Collimated Outflows Limits Accretion onto Massive Stars

Most massive stars are in binaries, but where do they go after becoming magnetars? :
- Where are the magnetar binary companions? Candidates from a comparison with binary population synthesis predictions

Young stars and leaking Lyman photons:
- The VANDELS survey: a measurement of the average Lyman-continuum escape fraction of star-forming galaxies at z=3.5