Beta Pictoris is an A-type star hosting a complex planetary system with two massive gas giants and a prominent debris disk.
Beta PIctoris
Multi-modal Atmospheric Characterization Of beta Pictoris b: Adding High-resolution Continuum Spectra From GRAVITY
We present the first VLTI/GRAVITY observations at Rλ∼4000 of β Pic b. These four high S/N (∼20) K-band spectra conserve both the pseudo-continuum and molecular absorption patterns.
Exocomets of Beta Pictoris I: Exocomet destruction, sodium and disk line variability in 17 years of HARPS observations
The young β Pictoris system has been monitored with high-resolution optical spectrographs for decades. These observations have revealed strongly variable absorption in the Ca II H\&K lines attributed to in-falling […]
Abundances Of Refractory Ions In Beta Pictoris Exocomets
Beta Pic is a young, A5V star, known for harbouring a large number of exocomets, which frequently transit the star and produce absorption signatures.
Dynamics of the Beta Pictoris Planetary System and Possibility of an Additional Planet
The Beta Pictoris system is characterized by a dusty debris disk, in addition to the presence of two already known planets. This makes it a particularly interesting case for studying […]
Deep High-resolution L Band Spectroscopy In The B Pictoris Planetary System
The beta Pictoris system, with its two directly imaged planets beta Pic b and beta Pic c and its well characterised debris disk, is a prime target for detailed characterisation […]
Detection And Characterisation Of Giant Planets With Gaia Astrometry
Astrometric observations with Gaia are expected to play a valuable role in future exoplanet surveys. With current data from Gaia’s third data release (DR3), we are sensitive to periods from […]
Numerical Simulations of Exocomet Transits: Insights From BetaPic and KIC 3542116
In recent years, the topic of existence and exploration of exocomets has been gaining increasing attention. The asymmetrical decrease in the stellar brightness due to the passage of a comet-like […]
Into The Red: An M-band Study of the Chemistry and Rotation of β Pictoris b at High Spectral Resolution
High-resolution cross-correlation spectroscopy (HRCCS) combined with adaptive optics has been enormously successful in advancing our knowledge of exoplanet atmospheres, from chemistry to rotation and atmospheric dynamics.
Curves Of Growth For Transiting Exocomets: Application To Fe II Lines In The Beta Pictoris System
This study introduces the exocomet curve of growth, a new method to analyse the variable absorptions observed in β Pictoris spectrum and link them to the physical properties of the […]
