Results 151 to 160 of about 89,333 (270)

Outflows from the youngest stars are mostly molecular. [PDF]

open access: yesNature, 2023
Ray TP   +22 more
europepmc   +1 more source

The Spitzer c2d Survey of Large, Nearby, Interstellar Clouds. I. Chamaeleon II Observed with MIPS

open access: yes, 2005
We present maps of over 1.5 square degrees in Chamaeleon (Cha) II at 24, 70, and 160 micron observed with the Spitzer Space Telescope Multiband Imaging Photometer for Spitzer (MIPS) and a 1.2 square degree millimeter map from SIMBA on the Swedish-ESO ...
Alcala', J.   +22 more
core   +1 more source

A new era in solar system astronomy with JWST. [PDF]

open access: yesNat Commun, 2023
Villanueva GL, Milam SN.
europepmc   +1 more source

First Mid‐Infrared Spectrum of a Faint High‐ z Galaxy: Observations of CFRS 14.1157 with the Infrared Spectrograph on the Spitzer Space Telescope [PDF]

open access: bronze, 2004
S. J. U. Higdon   +9 more
openalex   +1 more source

Spitzer Space Telescope Observations of Circumbinary Dust Disks around Polars [PDF]

open access: yes, 2007
We present Spitzer Space Telescope IRAC photometry of the magnetic cataclysmic variables EF Eri, MR Ser, VV Pup, V834 Cen, GG Leo and V347 Pav. When we combine our results with the 2MASS data, we find that at least five of the polars have flux densities ...
Brinkworth, C. S.   +8 more
core  

The state of the focus and image quality of the Spitzer Space Telescope as measured in orbit [PDF]

open access: green, 2004
R. D. Gehrz   +13 more
openalex   +1 more source

Analysis of the Full Spitzer Microlensing Sample. I. Dark Remnant Candidates and Gaia Predictions

open access: yesThe Astrophysical Journal
In the pursuit of understanding the population of stellar remnants within the Milky Way, we analyze the sample of ∼950 microlensing events observed by the Spitzer Space Telescope between 2014 and 2019.
Krzysztof A. Rybicki   +76 more
doaj   +1 more source

The Baryonic Tully–Fisher Relation. II. Stellar Mass Models

open access: yesThe Astronomical Journal
We present new color–ϒ _* (mass-to-light ratio) models to convert Wide-field Infrared Survey Explorer W1 fluxes into stellar masses. We outline a range of possible star formation histories and chemical evolution scenarios to explore the confidence limits
Francis Duey   +3 more
doaj   +1 more source

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