[astro-ph.EP] High resolution imaging with optical speckle interferometry has revealed that many transiting exoplanet host stars possess close-in stellar companions.
stellar cartogaphy
Life 2.0: A Scalable Distributed Space-Telescope Array For Biosignature Spectroscopy
[astro-ph.IM] Answering the question “Are we alone?” requires atmospheric spectroscopy of nearby terrestrial planets. For an Earth–Sun analog, even the strongest transmission signals are expected to be of order 1 […]
The Pan-Pacific Planet Search — IX. A Menagerie Of Companions Orbiting Evolved Stars
We present resolutions as to the nature of six speculative candidate companions proposed in the final data release of the Pan-Pacific Planet Search, a 6-year radial-velocity survey of 164 southern […]
Astronomers Find Missing Link To Our Galaxy’s Most Common Planets
One of the biggest recent surprises in astronomy is the discovery that most stars like the Sun harbor a planet between the size of Earth and Neptune within the orbit […]
Precise Physical Parameters, Habitability, and Orbital Stability of Sun-like SB2 Systems: HD 130669, HD 184467, HD 191854, and HD 214222
This work analyzes four Sun-like double-lined spectroscopic binary (SB2) systems by combining visual and spectroscopic observational data with Al-Wardat’s atmospheric modeling method to accurately determine their fundamental parameters.
Stellar Flares In The TESS Light Curves Of Planet-hosting M dwarfs
M dwarfs are magnetically active stars that frequently produce flares, which have implications for both stellar evolution and exoplanet studies.
