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- W1981121489 abstract "view Abstract Citations (11) References (31) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Velocity Structure in Optical CH + Lines toward HD 190603 and Implications for the Formation of CH + Allen, M. M. ; Snow, Theodore P. Abstract Observations of CH(+) and other species accessible in optical wavelengths in the line of sight to HD 190603, a B 1.5 Iae supergiant are reported. In this line of sight a shift in radial velocity between the CH(+) line and other interstellar absorption lines such as CH and Ca I is observed. The most likely explanation for this effect is the shock formation of CH(+). Likely preshock and postshock conditions which are consistent with the observations are also estimated. Publication: The Astrophysical Journal Pub Date: May 1992 DOI: 10.1086/171333 Bibcode: 1992ApJ...391..152A Keywords: B Stars; Hydrocarbons; Interstellar Chemistry; Line Spectra; Stellar Spectra; Supergiant Stars; Absorption Spectra; Abundance; Reflection Nebulae; Shock Waves; Visible Spectrum; Astrophysics; ISM: MOLECULES; SHOCK WAVES; STARS: INDIVIDUAL HENRY DRAPER NUMBER: HD 190603 full text sources ADS | data products SIMBAD (1)" @default.
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- W1981121489 date "1992-05-01" @default.
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- W1981121489 title "Velocity structure in optical CH(+) lines toward HD 190603 and implications for the formation of CH(+)" @default.
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