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The interstellar carbon abundance. II - Rho Ophiuchi and Beta Scorpii (1986)

Hobbs, L. M. ; York, D. G. ; Welty, D. E.

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Publication Date: 2019-07-12

Description: A procedure designed to obtain increased sensitivity from high-dispersion IUE spectra by using a flat-field spectrum to remove nonrandom noise due to the response pattern of the SEC vidicon detector is described. Application of this procedure to spectra of Rho Oph and Beta(1) Sco near the spin-forbidden interstellar 2325 line of C II yields 2 sigma upper limits on absorption of W (lambda) not greater than about 4 mA. The resulting depletion of carbon from the interstellar gas toward Rho Oph exceeds a factor of 1.4.

Keywords: ASTROPHYSICS

Type: Astronomical Society of the Pacific, Publications (ISSN 0004-6280); 98; 857-861

Format: text

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