JHKLM photometry for carbon stars

@article{Taranova2004JHKLMPF,
  title={JHKLM photometry for carbon stars},
  author={O. Taranova and V. Shenavrin},
  journal={Astronomy Letters},
  year={2004},
  volume={30},
  pages={549-565}
}
We discuss our JHKLM photometry for nine carbon Mira stars, eighteen carbon semiregular variables, and two oxygen Mira stars. For fourteen carbon stars, we present and analyze their infrared light and color curves. For all of the observed objects, we have estimated the optical depths of the circumstellar dust envelopes, the angular diameters of the stars, and their temperatures. 
View on Springer
9 Citations
Background Citations
2
Methods Citations
1

9 Citations

Citation Type

Citation Type

IR photometry and models for the dust envelopes of two carbon stars
IR photometry and dust-shell models for two carbon stars
IR photometry and a model of a dust shell in V2108 Ophiuchi
Infrared spectral variations of three Mira variable carbon stars with the 11.3 μm SiC feature
  • 2
Near-infrared observations of the carbon stars TU Geminorum and SS Virginis at milliarcsecond resolution
  • 2
  • PDF
AGB variables and the Mira period–luminosity relation
  • 166
  • PDF
Carbon-rich Mira variables: radial velocities and distances
  • 28
  • PDF
The Radiative Pattern and Asymmetry of IRC +10216 at 11 μm Measured with Interferometry and Closure Phase
  • 7
  • PDF
A Model of the Dust Envelope of the Carbon Mira Star V CrB from Photometry, Infrared Spectroscopy, and Speckle Polarimetry
  • 1