[HTML][HTML] The determination of ultraviolet extinction from the optical and near-infrared
JA Cardelli, GC Clayton…�- …�), vol. 329, June 1, 1988, p�…, 1988 - adsabs.harvard.edu
… techniques to two lines of sight with extremely peculiar extinction curves, HD 62542 and HD
29647 (Cardelli … Some weak correlations will be discussed in Cardelli, Clayton, and Mathis …
29647 (Cardelli … Some weak correlations will be discussed in Cardelli, Clayton, and Mathis …
The relationship between IR, optical, and UV extinction
JA Cardelli, GC Clayton, JS Mathis�- NASA, Ames Research Center�…, 1989 - ntrs.nasa.gov
An analysis is presented for the variability of absolute IR, optical, and UV extinction, A(sub
lambda), derived through the ratio of total-to-selective extinction, R, for 31 lines of sight for …
lambda), derived through the ratio of total-to-selective extinction, R, for 31 lines of sight for …
[HTML][HTML] Polarization and the ratio of total-to-selective extinction
GC Clayton, JA Cardelli�- …�Journal (ISSN 0004-6256), vol. 96�…, 1988 - adsabs.harvard.edu
… are quadratic functions of 2 1 (Cardelli, Clayton, and … sight have differing extinction
laws even in the visual (Cardelli and Clayton 1988; Cardelli, Clayton, and Mathis … This�…
laws even in the visual (Cardelli and Clayton 1988; Cardelli, Clayton, and Mathis … This�…
[HTML][HTML] Absolute extinction and the influence of environment-Dark cloud sight lines toward VCT 10, 30, and Walker 67
JA Cardelli, GC Clayton�- …�Journal (ISSN 0004-6256), vol. 101�…, 1991 - adsabs.harvard.edu
The range of validity of the average absolute extinction law (AAEL) proposed by Cardelli et
al.(1988 and 1989) is investigated, combining published visible and NIR data with IUE UV …
al.(1988 and 1989) is investigated, combining published visible and NIR data with IUE UV …
[PDF][PDF] The parameter R, seems well related to the strength of the A2175 bump but not to the central wavelength or the width of the bump. The dependence of the “far�…
JA CARDELLI, GC CLAYTON, JS MATHIS - astrowww.phys.uvic.ca
… Deviations on the extinction at 0.13 pum appear to be highly correlated with deviations at
0.17 pum (Cardelli and Mathis 1989). Our results call into question the reasoning of GC that if …
0.17 pum (Cardelli and Mathis 1989). Our results call into question the reasoning of GC that if …
[HTML][HTML] Abundance of interstellar carbon toward Zeta Ophiuchi
JA Cardelli, JS Mathis, DC Ebbets…�- …�, vol. 402, no. 1, p. L17�…, 1993 - adsabs.harvard.edu
We report on the detection of the weak intersystem transition of semiforbidden C II 2325 A in
the sight line toward Zeta Oph using the Ech-B mode of the Goddard High-Resolution …
the sight line toward Zeta Oph using the Ech-B mode of the Goddard High-Resolution …
[HTML][HTML] The relationship between infrared, optical, and ultraviolet extinction
JA Cardelli, GC Clayton…�- …�), vol. 345, Oct. 1, 1989, p�…, 1989 - adsabs.harvard.edu
… come from the list given in Clayton and Cardelli (1988). As … At first glance our results
seem at variance with those of GC, … Deviations on the extinction at 0.13 ~um appear to be�…
seem at variance with those of GC, … Deviations on the extinction at 0.13 ~um appear to be�…
Can CCM law properly represent all extinction curves?
A Geminale, P Popowski�- Journal of Physics: Conference Series, 2005 - iopscience.iop.org
… We derive total to selective extinction ratios based on the Cardelli, Clayton & Mathis (1989,
CCM) law, which is typically used to fit the extinction data both for diffuse and dense …
CCM) law, which is typically used to fit the extinction data both for diffuse and dense …
Ultraviolet extinction properties in the Milky Way
LA Valencic, GC Clayton, KD Gordon�- The Astrophysical Journal, 2004 - iopscience.iop.org
… We find that (1) the Cardelli, Clayton, & Mathis (CCM) extinction law applies for 93% of
the sight lines, implying that dust processing in the Galaxy is efficient and systematic, (2) the …
the sight lines, implying that dust processing in the Galaxy is efficient and systematic, (2) the …
[HTML][HTML] Interstellar molecular lines in the direction of the young star TY CrA
JA Cardelli, G Wallerstein�- …�Journal (ISSN 0004-6256), vol. 97�…, 1989 - adsabs.harvard.edu
… Cardelli and Wallerstein (1986) attributed this difference to … same observing run as the
Cardelli and Wallerstein data, the … Ax/Av vs Rv~1 relationship of Cardelli, Clayton, and Mathis …
Cardelli and Wallerstein data, the … Ax/Av vs Rv~1 relationship of Cardelli, Clayton, and Mathis …