Measuring Galactic Extinction: A Test
暂无分享,去创建一个
[1] D. Schlegel,et al. Maps of Dust Infrared Emission for Use in Estimation of Reddening and Cosmic Microwave Background Radiation Foregrounds , 1998 .
[2] D. Schlegel,et al. Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds , 1997, astro-ph/9710327.
[3] P. Myers,et al. IRAS images of nearby dark clouds , 1994 .
[4] L. Hartmann,et al. A new optical extinction law and distance estimate for the Taurus-Auriga molecular cloud , 1994 .
[5] Elizabeth A. Lada,et al. Dust Extinction and Molecular Gas in the Dark Cloud IC 5146 , 1994 .
[6] W. Herbst,et al. Far-infrared emission in the Rho Ophiuchi region - A comparison with molecular gas emission and visual extinction , 1989 .
[7] S. Faber,et al. Spectroscopy and Photometry of Elliptical Galaxies. VI. Sample Selection and Data Summary: Erratum , 1989 .
[8] F. Vrba,et al. On the ratio of total-to-selective extinction in the Taurus dark cloud complex , 1985 .
[9] C. Heiles,et al. Reddenings derived from H I and galaxy counts : accuracy and maps. , 1982 .
[10] C. Heiles,et al. H I, galaxy counts, and reddening: Variation in the gas-to-dust ratio, the extinction at high galactic latitudes, and a new method for determining galactic reddening , 1978 .