Zobrazeno 1 - 10
of 85
pro vyhledávání: '"Price, Stephan D."'
Autor:
Ryan, Erin Lee, Mizuno, Donald R., Shenoy, Sachindev S., Woodward, Charles E., Carey, Sean, Noriega-Crespo, Alberto, Kraemer, Kathleen E., Price, Stephan D.
Multi-epoch Spitzer Space Telescope 24 micron data is utilized from the MIPSGAL and Taurus Legacy surveys to detect asteroids based on their relative motion. These infrared detections are matched to known asteroids and rotationally averaged diameters
Externí odkaz:
http://arxiv.org/abs/1204.1116
Autor:
Kraemer, Kathleen E., Hora, Joseph L., Egan, Michael P., Adams, Joseph, Allen, Lori E., Bontemps, Sylvain, Carey, Sean J., Fazio, Giovanni G., Gutermuth, Robert, Keto, Eric, Koenig, Xavier P., Megeath, S. Thomas, Mizuno, Donald R., Motte, Frederique, Price, Stephan D., Schneider, Nicola, Simon, Robert, Smith, Howard
We present observations of newly discovered 24 micron circumstellar structures detected with the Multiband Imaging Photometer for Spitzer (MIPS) around three evolved stars in the Cygnus-X star forming region. One of the objects, BD+43 3710, has a bip
Externí odkaz:
http://arxiv.org/abs/1003.2437
Autor:
Uttenthaler, Stefan, Stute, Matthias, Sahai, Raghvendra, Blommaert, Joris A. D. L., Schultheis, Mathias, Kraemer, Kathleen E., Groenewegen, Martin A. T., Price, Stephan D.
Aims: We aim at measuring mass-loss rates and the luminosities of a statistically large sample of Galactic bulge stars at several galactocentric radii. The sensitivity of previous infrared surveys of the bulge has been rather limited, thus fundamenta
Externí odkaz:
http://arxiv.org/abs/1002.5015
Autor:
Kraemer, Kathleen E., Sloan, G. C., Bernard-Salas, J., Price, Stephan D., Egan, Michael P., Wood, P. R.
Publikováno v:
Astrophys.J.652:L25-L28,2006
We have observed an evolved star with a rare combination of spectral features, MSX SMC 029, in the Small Magellanic Cloud (SMC) using the low-resolution modules of the Infrared Spectrograph on the Spitzer Space Telescope. A cool dust continuum domina
Externí odkaz:
http://arxiv.org/abs/astro-ph/0611127
Publikováno v:
Astrophys.J.631:L147-L150,2005
We observed 36 evolved stars in the Small Magellanic Cloud (SMC) using the low-resolution mode of the Infrared Spectrograph (IRS) on the Spitzer Space Telescope. Two of these stars, MSX SMC 014 and 155, have nearly featureless spectral energy distrib
Externí odkaz:
http://arxiv.org/abs/astro-ph/0509507
Publikováno v:
Astron.J.131:612-620,2006
To search for phase lags in the optical-infrared light curves of asymptotic giant branch stars, we have compared infrared data from the COBE DIRBE satellite with optical light curves from the AAVSO and other sources. We found 17 examples of phase lag
Externí odkaz:
http://arxiv.org/abs/astro-ph/0509204
We present the COBE DIRBE Point Source Catalog, an all-sky catalog containing infrared photometry in 10 bands from 1.25 microns to 240 microns for 11,788 of the brightest near and mid-infrared point sources in the sky. Since DIRBE had excellent tempo
Externí odkaz:
http://arxiv.org/abs/astro-ph/0406177
Publikováno v:
Astrophys.J.Suppl. 140 (2002) 389
The Infrared Space Observatory observed over 900 objects with the Short Wavelength Spectrometer in full-grating-scan mode (2.4-45.2 micron). We have developed a comprehensive system of spectral classification using these data. Sources are assigned to
Externí odkaz:
http://arxiv.org/abs/astro-ph/0201507
Publikováno v:
565: L55-L58, 2002 January 20
Spectra from the Short Wavelength Spectrometer (SWS) on ISO exhibit artifacts at 4.5 and 8 um. These artifacts appear in spectra from a recent data release, OLP 10.0, as spurious broad emission features in the spectra of stars earlier than ~F0, such
Externí odkaz:
http://arxiv.org/abs/astro-ph/0112447
Publikováno v:
Astron.J. 122 (2001) 1844-1860
The Large Magellanic Cloud (LMC) has been observed by both the Midcourse Space Experiment (MSX) in the mid-infrared and the Two Micron All Sky Survey (2MASS) in the near-infrared. We have performed a cross-correlation of the 1806 MSX catalog sources
Externí odkaz:
http://arxiv.org/abs/astro-ph/0107220