We present JWST/MIRI observations of the debris disk surrounding the nearby, solar analog Epsilon Eridani obtained as part of the Archetypal Debris Disk GTO program.
Epsilon Eridani
Direct Imaging For The Debris Disk Around epsilon Eridani With The Cool-Planet Imaging Coronagraph
We analyze the inner debris disk around ϵ Eridani using simulated observations with the Cool-Planet Imaging Coronagraph (CPI-C).
Searching For Planets Orbiting Epsilon Eridani With JWST/NIRCam
We present observations of ϵ Eridani with the JWST/NIRCam coronagraph aimed at imaging planets orbiting within this system.
Revised Mass and Orbit of Epsilon Eridani b: A 1 Jupiter-Mass Planet on a Near-Circular Orbit
The mature Jovian planet ε Eridani b orbits one of the closest sun-like stars at a moderate separation of 3.5 AU, presenting one of the best opportunities to image a […]
Deepest Limits On Scattered Light Emission From The Epsilon Eridani Inner Debris Disk With HST/STIS
Epsilon Eridani (ϵ Eri) is one of the first debris disk systems detected by the Infrared Astronomical Satellite (IRAS).
SPHERE RefPlanets: Search For Epsilon Eridani b And Warm Dust
We carried out very deep VLT/SPHERE imaging polarimetry of the nearby system Eps Eri based on 38.5 hours of integration time with a 600 – 900 nm broadband filter to […]
Stellar Winds Of Three Sun-like Stars Detected For The First Time
An international research team led by a researcher from the University of Vienna has for the first time directly detected stellar winds from three Sun-like stars by recording the X-ray […]
Imaging Of Exocomets With Infrared Interferometry
Active comets have been detected in several exoplanetary systems, although so far only indirectly, when the dust or gas in the extended coma has transited in front of the stellar […]
The Crucial Role Of Surface Magnetic Fields For Stellar Dynamos: Epsilon Eridani, 61 Cygni A, and the Sun
Cool main-sequence stars, such as the Sun, have magnetic fields which are generated by an internal dynamo mechanism. In the Sun, the dynamo mechanism produces a balance between the amounts […]
An Application Of A solar-type Dynamo Model For Epsilon Eridani
During the last decade, the relation between activity cycle periods with stellar parameters has received special attention. The construction of reliable registries of activity reveals that solar type stars exhibit […]
