TY - JOUR
T1 - Detection of boron, cobalt, and other weak interstellar lines toward ζ ophiuchi
AU - Federman, S. R.
AU - Sheffer, Y.
AU - Lambert, D. L.
AU - Gilliland, R. L.
N1 - Copyright:
Copyright 2018 Elsevier B.V., All rights reserved.
PY - 1993/8/10
Y1 - 1993/8/10
N2 - Numerous weak lines from interstellar atomic species toward ζ Ophiuchi were observed with the Goddard High-Resolution Spectrograph. Of particular note are the first interstellar detection of cobalt and the detection of boron in this sight line. These measurements provide estimates for the amount of depletion for the two elements. Boron, a volatile, and cobalt, a refractory element, display the depletion pattern found by Savage, Cardelli, & Sofia (1992). The abundance of phosphorus in the H II region associated with the star was obtained from a detection of P III. Additional weak lines from S I, C I, Ni II, and Cu II were detected for the first time; these lines provide the basis for refinements in oscillator strength and column density. Analysis of the neutral sulfur data indicates that the atomic gas is more widely distributed than the molecular material in the main component.
AB - Numerous weak lines from interstellar atomic species toward ζ Ophiuchi were observed with the Goddard High-Resolution Spectrograph. Of particular note are the first interstellar detection of cobalt and the detection of boron in this sight line. These measurements provide estimates for the amount of depletion for the two elements. Boron, a volatile, and cobalt, a refractory element, display the depletion pattern found by Savage, Cardelli, & Sofia (1992). The abundance of phosphorus in the H II region associated with the star was obtained from a detection of P III. Additional weak lines from S I, C I, Ni II, and Cu II were detected for the first time; these lines provide the basis for refinements in oscillator strength and column density. Analysis of the neutral sulfur data indicates that the atomic gas is more widely distributed than the molecular material in the main component.
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U2 - 10.1086/186957
DO - 10.1086/186957
M3 - Article
AN - SCOPUS:12044256570
SN - 0004-637X
VL - 413
SP - L51-L54
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 1 PART 2
ER -