Results 31 to 40 of about 85 (81)
We report on coronagraphic observations of the nearest solar-type star, α Centauri A ( α Cen A), using the MIRI instrument on the James Webb Space Telescope.
Charles Beichman +29 more
doaj +1 more source
The James Webb Space Telescope (JWST) observed our closest solar twin, α Centauri A ( α Cen A), with the Mid-Infrared Instrument in the F1550C (15.5 μ m) coronagraphic imaging mode at three distinct epochs between 2024 August and 2025 April.
Aniket Sanghi +16 more
doaj +1 more source
FIRST-LIGHT LBT NULLING INTERFEROMETRIC OBSERVATIONS: WARM EXOZODIACAL DUST RESOLVED WITHIN A FEW AU OF η Crv [PDF]
9 pages, 6 figures, accepted for publication in ...
Defrere, Denis +39 more
openaire +4 more sources
How Long-lived Grains Dominate the Shape of the Zodiacal Cloud
Grain–grain collisions shape the three-dimensional size and velocity distribution of the inner Zodiacal Cloud and the impact rates of dust on inner planets, yet they remain the least understood sink of zodiacal dust grains. For the first time, we combine
Petr Pokorný +4 more
doaj +1 more source
EXOZODIACAL DUST LEVELS FOR NEARBY MAIN-SEQUENCE STARS: A SURVEY WITH THE KECK INTERFEROMETER NULLER [PDF]
The Keck Interferometer Nuller (KIN) was used to survey 25 nearby main-sequence stars in the mid-infrared, in order to assess the prevalence of warm circumstellar (exozodiacal) dust around nearby solar-type stars. The KIN measures circumstellar emission by spatially blocking the star but transmitting the circumstellar flux in a region typically 0.1-4 ...
Millan-Gabet, R. +14 more
openaire +2 more sources
JWST/NIRSpec Detects Warm CO Emission in the Terrestrial-planet Zone of HD 131488
We have obtained a high-resolution, JWST NIRSpec 2.87–5.14 μ m spectrum of the debris disk around HD 131488. We discover CO fundamental emission indicating the presence of warm fluorescent gas within ∼10 au of the star.
Cicero X. Lu +14 more
doaj +1 more source
Hot exozodiacal dust around Fomalhaut: The MATISSE perspective
Context. Excess over the stellar photospheric emission of main-sequence stars has been found in interferometric near-infrared observations, and is attributed to the presence of hot exozodiacal dust (HEZD). As part of our effort to detect and characterize HEZD around the nearby A3 V star Fomalhaut, we carried out the first interferometric observations ...
K. Ollmann +8 more
openaire +2 more sources
Prospects for the characterisation of exo-zodiacal dust with the VLTI [PDF]
Accepted for publication in Experimental ...
Ertel, S. +4 more
openaire +6 more sources
The HOSTS survey for exo-zodiacal dust: preliminary results and future prospects [PDF]
[abridged] The presence of large amounts of dust in the habitable zones of nearby stars is a significant obstacle for future exo-Earth imaging missions. We executed an N band nulling interferometric survey to determine the typical amount of such exozodiacal dust around a sample of nearby main sequence stars.
Ertel, S. +42 more
openaire +4 more sources
The dynamics of exozodiacal dust
This thesis manuscript presents the work that I carried out during my thesis, the subject of which is "The dynamics of exozodiacal dust".The exozodiacal dust, is, by analogy to the zodiacal dust of the solar system, the internal component of debris disks around stellar systems : dust located from a few stellar radii to few astronomical units.
openaire +1 more source

