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ASOCAM Observations of CYG X-3: Search for a Hot Stellar Wind

Fender, R. P.; Ogley, R. N.; Burnell, S. J. Bell

Six CAM observations have been made in the 4 - 14 µm wavelength region to search for further evidence of emission from a hot stellar wind. Initial results suggest that the spectrum detected by Fender et al. using UKIRT extends into the wavelength region covered by ISOCAM. There is also evidence that the source is variable on timescales of ≈ 70 sec…

Calibration of the Debris Project ISOPHOT Data

Silverstone, Murray; Becklin, E. E.; Spangler, Celeste

Analysis of Infrared Spectra of Carbon Stars Observed by the ISO SWS

Ohnaka, K.; Yamamura, I.; Tsuji, T. +1 more

Blue Compact Galaxies at Redshifts Z=0.2-1.3

Guzmán, R.

We study the nature of faint blue compact galaxies (BCGs) at redshifts z ∼ 0.2 - 1.3 using Keck and HST. Despite being very luminous (L_B ∼ L^*), most distant BCGs have masses M ∼ 10¹⁰M_⊙, i.e., they are dwarf stellar systems. The majority of these galaxies have colors, sizes, surface brightnesses, luminosi…

Evolution and Mass Loss of AGB Stars in the Small Magellanic Cloud

Waters, L. B. F. M.; Blommaert, J. A. D. L.; van Loon, J. Th. +7 more

Clues to the Evolution of Massive Stars from their Far-Infrared Environments

Marston, A. P.

ISO-SWS Spectral Characterization of Stars

Heras, A. M.; Shipman, R. F.; Price, S. D. +6 more

ISOPHOT Observations of VEGA and Vega-like Stars

Walker, H. J.; Heinrichsen, I.

Detailed ISOPHOT observations of the far infrared excess of α Lyrae (Vega) are presented. The data comprise photometry in the range 25µm to 200µm and high resolution 60µm scan data to compare with 60µm and 90µm oversampled maps. The dust disk around Vega is clearly resolved. In addition similar maps of HD98800, SAO226057, SAO186777 and α Piscis Au…

Molecular Features in ISO-SWS Spectra of O-Rich Long-Period Variables

Hron, J.; Kerschbaum, F.; Aringer, B. +1 more

ISO Spectroscopy of AGB Stars in the Magellanic Clouds

Waters, L. B. F. M.; Blommaert, J. A. D. L.; van Loon, J. Th. +7 more