Results 171 to 180 of about 63,480 (217)

Investigating the Absorption Properties of Pure and Nitrogen-Doped Carbon Clusters as Models for the Core of Carbon Nanodots. [PDF]

J Phys Chem A
D'Ambrosio F, Frustaci A, Azzali A, Bodo E.   +3 more
europepmc   +1 more source

Infrared Study of Electron-bombarded Phenanthrene (C₁₄H₁₀)/<i>Para</i>-H₂ Matrices: Isomers of Protonated Phenanthrene (1-, 3-, 4-, and 9-H⁺C₁₄H₁₀). [PDF]

J Phys Chem A
Feng JY, Lee YP.
europepmc   +1 more source

A nearby dark molecular cloud in the Local Bubble revealed via H₂ fluorescence. [PDF]

Nat Astron
Burkhart B, Dharmawardena TE, Bialy S, Haworth TJ, Cruz Aguirre F, Jo YS, Andersson BG, Chung H, Edelstein J, Grenier I, Hamden ET, Han W, Hoadley K, Lee MY, Min KW, Müller T, Pattle K, Peek JEG, Pleiss G, Schiminovich D, Seon KI, Wilson AG, Zucker C.   +22 more
europepmc   +1 more source

Spectrophotometry of interstellar absorption bands

, 1975
openaire   +1 more source

Analytical applications of gas-phase ion chemistry enabled by mass spectrometry.

Anal Methods
Kang WY, Prentice BM.
europepmc   +1 more source

Predicting accurate binding energies and vibrational spectroscopic features of interstellar icy species. A quantum mechanical study.

Phys Chem Chem Phys
Bulik A, Martínez-Bachs B, Bancone N, Mates-Torres E, Corno M, Ugliengo P, Rimola A.   +6 more
europepmc   +1 more source

The origin of unidentified interstellar absorption lines

, 1939
Swings, Polydore, Öhman, Y.
openaire   +1 more source

Interstellar absorption lines in the ultraviolet

, 1974
openaire   +1 more source

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Interstellar Silicate Absorption Bands

Nature, 1970
Interstellar silicate absorption is observed in the direction of the galactic centre. Most interstellar silicon seems to be in silicate form.
J A, Hackwell, R D, Gehrz, N J, Woolf
openaire   +4 more sources

Identification of the λ2, 200Å interstellar absorption feature

Nature, 1977
A BROAD absorption feature centred on λ2, 200A with a half-width of ∼ 300A appears in the spectra of reddened stars1–3. This conspicuous feature in the interstellar extinction curve, might hold an important clue to the identity of a major component of interstellar matter, but it has defied identification for over a decade. Here we identify this band as
F. Hoyle, N. C. Wickramasinghe
openaire   +3 more sources