Planets orbiting in the habitable zones of white dwarfs have recently been proposed as promising targets for biosignature searches.
Stellar Cartography
Radio Galaxy Zoo EMU: Harnessing Citizen Science and AI to Advance Open Science Catalogues
Over the past decades, significant efforts have been devoted to developing sophisticated algorithms for automatically identifying and classifying radio sources in large surveys.
Evolution of Stellar Activity and Habitable zone: I. Ultraviolet Emission of Dwarfs in Open Clusters and Field Stars
Near-ultraviolet (NUV) radiation from dwarf stars plays a critical role in shaping the habitability of planetary systems, yet its long-term evolution across different spectral types remains poorly investigated.
Seeking The Worlds Of Avatar: Prospects for Detecting Moons Orbiting a Giant Planet in Alpha Centauri A’s Habitable Zone
Nearby giant exoplanets offer an opportunity to search for moons (exomoons) orbiting them. Here, we present a simulation framework for investigating the possibilities of detecting exomoons via their astrometric signal […]
The Evolution Of Complex Organic Molecules During Star Formation
Complex organic molecules (COMs) are thought to be the precursors of pre-biotic molecules and are observed in many protostellar sources.
The Variable Radio Emission Of V830 Tau And Its Putative Planet
We report on the first moderate-length time-scale observations of a young stellar object (YSO) at microwave frequencies. V830 Tau was monitored over the course of eight days with the JVLA […]
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 […]
An Analysis Of The Radius Gap In A Sample Of Kepler, K2 And TESS Exoplanets Orbiting M Dwarf Stars
Planetary radii are derived for 218 exoplanets orbiting 161 M dwarf stars. Stellar radii are based on an analysis of APOGEE high-resolution near-IR spectra for a subsample of the M-dwarfs; […]
How Stellar Mass And Disc Size Shape The Formation And Migration Of Super-Earths
The occurrence rate of close-in super-Earths is higher around M-dwarfs compared to stars of higher masses.
Do White Dwarfs Sample Water-Rich Planetary Material?
Polluted white dwarfs offer a unique way to directly probe the compositions of exoplanetary bodies.
