Found: 11
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Neutral chlorine and molecular hydrogen at high redshift.
- Published in:
- Astronomy & Astrophysics / Astronomie et Astrophysique, 2015, v. 575, p. 1, doi. 10.1051/0004-6361/201425553
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- Article
Estimation of physical conditions in the cold phase of the interstellar medium in the sub-DLA system at z = 2.06 in the spectrum of the quasar J 2123-0050.
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- Astronomy Letters, 2016, v. 42, n. 3, p. 137, doi. 10.1134/S1063773716030038
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- Article
HD/H molecular clouds in the early Universe: The problem of primordial deuterium.
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- Astronomy Letters, 2010, v. 36, n. 11, p. 761, doi. 10.1134/S1063773710110010
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- Article
Cosmology and fundamental physics with the ELT-ANDES spectrograph.
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- Experimental Astronomy, 2024, v. 57, n. 1, p. 1, doi. 10.1007/s10686-024-09928-w
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- Article
Molecular hydrogen in absorption at high redshifts: Science cases for CUBES.
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- Experimental Astronomy, 2023, v. 55, n. 1, p. 223, doi. 10.1007/s10686-022-09843-y
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- Article
Directional radiation and photodissociation regions in molecular hydrogen clouds.
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- Astronomy Letters, 2009, v. 35, n. 3, p. 150, doi. 10.1134/S1063773709030025
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- Article
MALS discovery of a rare H I 21 cm absorber at z ∼ 1.35: Origin of the absorbing gas in powerful active galactic nuclei.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 687, p. 1, doi. 10.1051/0004-6361/202348464
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- Article
PKS 1413+135: OH and H I at z = 0.247 with MeerKAT.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2023, v. 671, p. 1, doi. 10.1051/0004-6361/202245482
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- Article
Proximate molecular quasar absorbers: Excess of damped H<sub>2</sub> systems at z<sub>abs</sub> ≈ z<sub>QSO</sub> in SDSS DR14.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2019, v. 627, p. 1, doi. 10.1051/0004-6361/201935371
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- Article
Dissecting cold gas in a high-redshift galaxy using a lensed background quasar.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2018, v. 619, p. N.PAG, doi. 10.1051/0004-6361/201833608
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- Article
H/HD molecular clouds in the early universe. An independent means of estimating the baryon density of the universe.
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- Astronomy Reports, 2015, v. 59, n. 2, p. 100, doi. 10.1134/S1063772915020031
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- Article