Results 101 to 110 of about 60,149 (264)
Our understanding of how exoplanets form and evolve relies on analyses of both the mineralogy of protoplanetary disks and their detailed structures; however, these key complementary aspects of disks are usually studied separately.
William Grimble +9 more
doaj +1 more source
The Supernova Legacy of Spitzer Space Telescope
The mid-infrared (mid-IR) range offers an obvious and advantageous choice in following the late-time evolution of supernovae (SNe). First, the peaks of their spectral energy distributions (SED) shift toward the IR after the photospheric phase; second, mid-IR observations are practically free of interstellar extinction, which is also an important factor
openaire +1 more source
Two Decades of Dust Evolution in SN 2005af through JWST, Spitzer, and Chemical Modeling
The evolution of dust in core-collapse supernovae (SNe), in general, is poorly constrained owing to a lack of infrared observations a few years after explosion. Most theories of dust formation in SNe heavily rely only on SN 1987A.
Arkaprabha Sarangi +22 more
doaj +1 more source
Shedding New Light on the 3C 273 Jet with theSpitzer Space Telescope [PDF]
Y. Uchiyama +9 more
openalex +1 more source
87th Annual Meeting of the Meteoritical Society 2025: Abstracts
Meteoritics &Planetary Science, Volume 60, Issue S1, Page 30-350, August 2025.
wiley +1 more source
Solar system observations with Spitzer Space Telescope: Preliminary results [PDF]
The programs of observations of Solar System bodies conducted in the first year of the operation of the Spitzer Space Telescope as part of the Guaranteed Observing Time allocations are described. Initial results include the determination of the albedos of a number of Kuiper Belt objects and Centaurs from observations of their flux densities at 24 and ...
openaire +1 more source
An Improved Atlas of Full-scan Spectra from ISO/SWS
We present an atlas of full-scan spectra from the Short-Wavelength Spectrometer (SWS) on board the Infrared Space Observatory after reprocessing and improving an earlier version published 22 yr ago. The SWS spectra cover the wavelength range from 2.35 to
D. R. Mizuno +6 more
doaj +1 more source
Planetary nebulae detected in the Spitzer Space Telescope GLIMPSE 3D Legacy Survey [PDF]
Yong Zhang +4 more
openalex +1 more source
86th Annual Meeting of the Meteoritical Society (2024)
Meteoritics &Planetary Science, Volume 59, Issue S1, Page A1-A468, August 2024.
wiley +1 more source
Spitzer space telescope observatory planning and scheduling team
Launched as the space infrared telescope facility (SIRTF) in August, 2003 and renamed in early 2004, the Spitzer space telescope is performing an extended series of science observations at wavelengths ranging from 3 to 180 microns. The California Institute of Technology is the home of the Spitzer Science Center (SSC) and operates the science operations
Barba, Stephen J. +6 more
openaire +2 more sources

