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20 papers
Characterizing the Population of Bright Infrared Sources in the Small Magellanic Cloud
K. E. Kraemer, G. C. Sloan, P. R. Wood +2
We used Spitzer's Infrared Spectrograph (IRS) to observe stars in the Small Magellanic Cloud (SMC) selected from the Midcourse Space Experiment (MSX) Point Source Catalog. We conce…
An atlas of bright star spectra in the near infrared from Cassini-VIMS
Paul N. Stewart, Peter G. Tuthill, Philip D. Nicholson +2
We present the Cassini Atlas Of Stellar Spectra (CAOSS), comprised of near-infrared low-resolution spectra of bright stars recovered from space-based observations by the Cassini sp…
CASSIS: The Cornell Atlas of Spitzer/Infrared Spectrograph Sources. II. High-resolution observations
V. Lebouteiller, D. J. Barry, C. Goes +5
The Infrared Spectrograph (IRS) on board the Spitzer Space Telescope observed about 15,000 objects during the cryogenic mission lifetime. Observations provided low-resolution (R~60…
Spitzer Infrared Spectrographic point source classification in the Small Magellanic Cloud
Paul M. E. Ruffle, F. Kemper, O. C. Jones +16
The Magellanic clouds are uniquely placed to study the stellar contribution to dust emission. Individual stars can be resolved in these systems even in the mid-infrared, and they a…
Interstellar and circumstellar fullerenes
J. Bernard-Salas, J. Cami, A. P. Jones +6
Fullerenes are a particularly stable class of carbon molecules in the shape of a hollow sphere or ellipsoid that might be formed in the outflows of carbon stars. Once injected into…
VISTA variables in the Sagittarius dwarf spheroidal galaxy: pulsation- vs. dust-driven winds on the giant branches
Iain McDonald, Albert A. Zijlstra, Gregory C. Sloan +3
Variability is examined in over 2.6 million stars covering 11 square degrees of the core of the Sagittarius dwarf spheroidal galaxy (Sgr dSph) from VISTA Z-band observations. Gener…