Despite its biogenic and astrochemical importance, sulfur (S), the 10th most abundant element in the interstellar medium (ISM) with a total abundance of S/H ≈ 2.2 × 10 ^−5 , largely remains undetected in molecular clouds.
X. J. Yang, Lijun Hua, Aigen Li
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Recent Observations of Organic Molecules in Nearby Cold, Dark Interstellar Clouds [PDF]
Hiroshi Suzuki+7 more
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Molecular Deuterations in Massive Starless Clump Candidates
Deuterated molecules are valuable probes for investigating the evolution and the kinematics in the earliest stages of star formation. In this study, we conduct a comprehensive investigation by performing a single-point survey of 101 starless clump ...
Kai Yang+3 more
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Metal-containing molecules: some new candidates for interstellar detection [PDF]
Simon Petrie
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Ultraviolet Photoprocessing of Interstellar Dust Mantles as a Source of Polycyclic Aromatic Hydrocarbons and Other Conjugated Molecules [PDF]
J. Mayo Greenberg+8 more
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Appendix 2. Identified Interstellar and Circumstellar Molecules [PDF]
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On the detection of the linear C5 molecule in the interstellar medium [PDF]
Г. А. Галазутдинов+2 more
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Searches for new interstellar molecules, including a tentative detection of aziridine and a possible detection of propenal [PDF]
J. E. Dickens+7 more
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Assignment of the λ1369.13 Diffuse Interstellar Absorption Band and Three Other Far‐Ultraviolet Interstellar Absorption Lines to the CH Molecule [PDF]
J. K. G. Watson
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Structure, Spectroscopic Properties and Reactions of Interstellar Molecule HC2N and Isomers :Ab initio Study [PDF]
Sungwoo Park, Seong-Yul Lee
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