706 research outputs found
Some recent infrared spectroscopy of interstellar processes
The potential which infrared spectroscopic techniques provide for studying interstellar process is demonstrated. Several examples are given. The data were obtained at UKIRT, using its frequency-chopped Fabry-Perot spectrometer and its seven-channel cooled grating spectrometer
The Interstellar Medium of IRAS 08572+3915 NW: H3+ and Warm High Velocity CO
We confirm the first detection of the molecular ion H3+ in an extragalactic
object, the highly obscured ultraluminous galaxy IRAS 08572+3915 NW. We also
have detected absorption lines of the fundamental band of CO in this galaxy.
The CO absorption consists of a cold component close to the systemic velocity
and warm, highly blueshifted and redshifted components. The warm blueshifted
component is remarkably strong and broad and extends at least to -350 km/s.
Some analogies can be drawn between the H3+ and cold CO in IRAS08572+3915 NW
and the same species seen toward the Galactic center. The profiles of the warm
CO components are not those expected from a dusty torus of the type thought to
obscure active galactic nuclei. They are probably formed close to the dust
continuum surface near the buried and active nucleus and are probably
associated with an unusual and energetic event there.Comment: 21 pages, 4 postscript figures, accepted by Ap
The plumes of IO: A detection of solid sulfur dioxide particles
Spectra of Io obtained during eclipse show a narrow deep absorption feature at 4.871 microns, the wavelength of the Nu sub 1 + Nu sub 3 band of solid SO2. The 4 micron radiation comes from volcanic hot spots at a temperature too high for the existence of solid SO2. It is concluded that the spectral feature results from SO2 particles suspended in plumes above the hot spots. The derived abundance of approximately 0.0003 gm/sq cm may imply an SO2 solid-to-gas ratio of roughly one for the Loki plume, which would in turn suggest that it is driven by the SO2 rather than by sulfur
Variable Winds and Dust Formation in R Coronae Borealis Stars
We have observed P-Cygni and asymmetric, blue-shifted absorption profiles in
the He I 10830 lines of twelve R Coronae Borealis (RCB) stars over short (1
month) and long (3 year) timescales to look for variations linked to their
dust-formation episodes. In almost all cases, the strengths and terminal
velocities of the line vary significantly and are correlated with dust
formation events. Strong absorption features with blue-shifted velocities ~400
km/s appear during declines in visible brightness and persist for about 100
days after recovery to maximum brightness. Small residual winds of somewhat
lower velocity are present outside of the decline and recovery periods. The
correlations support models in which recently formed dust near the star is
propelled outward at high speed by radiation pressure and drags the gas along
with it.Comment: AJ in press, 21 pages, 3 figure
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