Results 91 to 100 of about 386,435 (271)

Mid-infrared spectroscopy of CAI and AOA from the Allende CV3.2 chondrite [PDF]

open access: yes, 2005
Mid-infrared spectra of bulk CAI from the CV3.2 chondrite Allende are presented and compared with astronomical spectra of cometary dust, zodiacal light,the circumstellar disk of beta Pictoris and dust around the red supergiant PR ...
Bland, P. A.   +5 more
core  

Herschel Observations of Dusty Debris Disks

open access: yes, 2016
We present results from two Herschel observing programs using the Photodetector Array Camera and Spectrometer. During three separate campaigns, we obtained Herschel data for 24 stars at 70, 100, and 160 microns.
Bryden, Geoff   +6 more
core   +1 more source

Post-AGB stars with hot circumstellar dust: binarity of the low-amplitude pulsators [PDF]

open access: yes, 2009
Context. The influence of binarity on the late stages of stellar evolut ion. Aims. While the first binary post-AGB stars were serendipitously d iscovered, the distinct characteristics of their Spectral Energy Distribution (SED) allowed us to launch a ...
H. Winckel   +30 more
semanticscholar   +1 more source

Electron microscopy observations of the diversity of Ryugu organic matter and its relationship to minerals at the micro‐ to nano‐scale

open access: yesMeteoritics &Planetary Science, Volume 59, Issue 8, Page 2023-2043, August 2024.
Abstract Transmission electron microscopy analyses of Hayabusa2 samples show that Ryugu organic matter exhibits a range of morphologies, elemental compositions, and carbon functional chemistries consistent with those of carbonaceous chondrites that have experienced low‐temperature aqueous alteration.
Rhonda M. Stroud   +112 more
wiley   +1 more source

The Dusty Aftermath of the V1309 Sco Binary Merger

open access: yes, 2013
We present mid-IR photometry and spectra of the merged binary V1309 Sco taken between 18 and 23 months after outburst. Strong mid-IR emission and a solid state absorption feature indicate the presence of a significant amount of dust in the circumstellar ...
Kozłowski, S.   +11 more
core   +1 more source

The New Class of Dusty DAZ White Dwarfs [PDF]

open access: yes, 2007
Our mid-infrared survey of 124 white dwarfs with the Spitzer Space Telescope and the IRAC imager has revealed an infrared excess associated with the white dwarf WD 2115-560 naturally explained by circumstellar dust.
Fergal Mullally   +7 more
core   +3 more sources

Hidden metallic iron in amorphous silicate dust?

open access: yesAstronomy & Astrophysics
Context. Amorphous silicate dust is a major component in the interstellar and circumstellar dust formed in the outflow of asymptotic giant branch (AGB) stars.
Enomoto H.   +3 more
doaj   +1 more source

A STUDY OF MASS LOSS AND DUST FORMATION NEAR HOT STARS

open access: yesOdessa Astronomical Publications, 2016
At present dust formation is well studied only near cool stars, whose surface temperatures are close to those of dust sublimation. Hot stars need to supply large amounts of circumstellar material to allow dust formation around them.
K. S. Kuratov   +6 more
doaj   +1 more source

Photophoretic Structuring of Circumstellar Dust Disks [PDF]

open access: yesThe Astrophysical Journal, 2008
We study dust accumulation by photophoresis in optically thin gas disks. Using formulae of the photophoretic force that are applicable for the free molecular regime and for the slip-flow regime, we calculate dust accumulation distances as a function of the particle size. It is found that photophoresis pushes particles (smaller than 10 cm) outward.
Takeuchi, Taku, Krauss, Oliver
openaire   +2 more sources

JWST imaging of the closest globular clusters—I. Possible infrared excess among white dwarfs in NGC 6397

open access: yesAstronomische Nachrichten, Volume 345, Issue 6-7, July-August 2024.
Abstract We present James Webb Space Telescope observations of the globular cluster NGC 6397 and use them to extend to infrared wavelengths the characterization of the cluster's entire white dwarf (WD) cooling sequence (CS). The data allows us to probe fundamental astrophysical WD properties and to search for evidence in their colors for (or against ...
L. R. Bedin   +11 more
wiley   +1 more source

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