Results 81 to 90 of about 3,801 (208)

Two Decades of Dust Evolution in SN 2005af through JWST, Spitzer, and Chemical Modeling

The Astrophysical Journal
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, Szanna Zsíros, Tamás Szalai, Laureano Martinez, Melissa Shahbandeh, Ori D. Fox, Schuyler D. Van Dyk, Alexei V. Filippenko, Melina Cecilia Bersten, Ilse De Looze, Chris Ashall, Tea Temim, Jacob E. Jencson, Armin Rest, Dan Milisavljevic, Luc Dessart, Eli Dwek, Nathan Smith, Samaporn Tinyanont, Thomas G. Brink, WeiKang Zheng, Geoffrey C. Clayton, Jennifer Andrews   +22 more
doaj   +1 more source

Trigger-Happy cloud

, 2011
This image combines data from X-ray Chandra Observatory and the Spitzer Telescope, and shows the star formation in a molecular cloud Cepheus B. The data from the Spitzer Telescope, red, green and blue, show the molecular cloud and new stars.
National Aeronautics and Space Administration (NASA), Jet Propulsion Laboratory, California Institute of Technology   +2 more
core   +1 more source

Trigger-Happy cloud

, 2016
This image combines data from X-ray Chandra Observatory and the Spitzer Telescope, and shows the star formation in a molecular cloud Cepheus B. The data from the Spitzer Telescope, red, green and blue, show the molecular cloud and new stars.
Jet Propulsion Laboratory, National Aeronautics and Space Administration (NASA), California Institute of Technology   +2 more
core   +1 more source

The Empirical and Radiative Transfer Hybrid (EaRTH) Disk Model: Merging Analyses of Protoplanetary Dust Disk Mineralogy and Structure

The Astrophysical Journal
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, Joel Kastner, Christophe Pinte, Beth Sargent, David A. Principe, Annie Dickson-Vandervelde, Aurora Belén Aguayo, Claudio Caceres, Matthias R. Schreiber, Keivan G. Stassun   +9 more
doaj   +1 more source

The Infrared Milky Way B

, 2016
Basic knowledge of AstronomyThis image was formed by the union of more than 444,000 images from NASA's Spitzer Space Telescope. It is possible to observe five components of the galactic plane, representing the formation of stars in our galaxyComponente ...
National Aeronautics and Space Administration (NASA), Jet Propulsion Laboratory, California Institute of Technology   +2 more
core   +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

An Improved Atlas of Full-scan Spectra from ISO/SWS

The Astrophysical Journal Supplement Series
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, T. A. Kuchar, Kathleen E. Kraemer, G. C. Sloan, Samantha Greene, Elianna Cohen, Holly Branco   +6 more
doaj   +1 more source

A Short and Personal History of the Spitzer Space Telescope

, 2005
12 pages, 3 figures; to appear in proceedings of "The Spitzer Space Telescope: New Views of the Cosmos"
openaire   +2 more sources

The Infrared Array Camera (IRAC) for the Spitzer Space Telescope

The Astrophysical Journal Supplement Series, 2004
The Infrared Array Camera (IRAC) is one of three focal plane instruments in the Spitzer Space Telescope. IRAC is a four-channel camera that obtains simultaneous broad-band images at 3.6, 4.5, 5.8, and 8.0 microns. Two nearly adjacent 5.2x5.2 arcmin fields of view in the focal plane are viewed by the four channels in pairs (3.6 and 5.8 microns; 4.5 and ...
G. G. Fazio, J. L. Hora, L. E. Allen, M. L. N. Ashby, P. Barmby, L. K. Deutsch, J.‐S. Huang, S. Kleiner, M. Marengo, S. T. Megeath, G. J. Melnick, M. A. Pahre, B. M. Patten, J. Polizotti, H. A. Smith, R. S. Taylor, Z. Wang, S. P. Willner, W. F. Hoffmann, J. L. Pipher, W. J. Forrest, C. W. McMurty, C. R. McCreight, M. E. McKelvey, R. E. McMurray, D. G. Koch, S. H. Moseley, R. G. Arendt, J. E. Mentzell, C. T. Marx, P. Losch, P. Mayman, W. Eichhorn, D. Krebs, M. Jhabvala, D. Y. Gezari, D. J. Fixsen, J. Flores, K. Shakoorzadeh, R. Jungo, C. Hakun, L. Workman, G. Karpati, R. Kichak, R. Whitley, S. Mann, E. V. Tollestrup, P. Eisenhardt, D. Stern, V. Gorjian, B. Bhattacharya, S. Carey, B. O. Nelson, W. J. Glaccum, M. Lacy, P. J. Lowrance, S. Laine, W. T. Reach, J. A. Stauffer, J. A. Surace, G. Wilson, E. L. Wright, A. Hoffman, G. Domingo, M. Cohen   +64 more
openaire   +2 more sources

The Infrared Milky Way A

, 2016
Basic knowledge of AstronomyThis image was formed by the union of more than 800,000 images from NASA's Spitzer Space Telescope. It is possible to observe five components of the galactic plane, representing a total of more than 50% of our Milky ...
National Aeronautics and Space Administration (NASA), Jet Propulsion Laboratory, California Institute of Technology   +2 more
core   +1 more source