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pro vyhledávání: '"H. Abgrall"'
Context. Highly excited molecular hydrogen H2 has been observed in many regions of shocked molecular gas. A recently published $K$-band spectrum of Herbig-Haro 7 (HH7) contains several vibration-rotation lines of H2 from highly excited energy levels
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2244ca55a78cb314fa4a8b629bab3645
http://arxiv.org/abs/2301.00741
http://arxiv.org/abs/2301.00741
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 450(2), 1237-1245. Oxford University Press
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2015, 450 (2), pp.1237-1245. ⟨10.1093/mnras/stv656⟩
Salumbides, E J, Bagdonaite, J, Abgrall, H, Roueff, E & Ubachs, W M G 2015, ' H-2 Lyman and Werner band lines and their sensitivity for a variation of the proton-electron mass ratio in the gravitational potential of white dwarfs ', Monthly Notices of the Royal Astronomical Society, vol. 450, no. 2, pp. 1237-1245 . https://doi.org/10.1093/mnras/stv656
Monthly Notices of the Royal Astronomical Society, 2015, 450 (2), pp.1237-1245. ⟨10.1093/mnras/stv656⟩
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2015, 450 (2), pp.1237-1245. ⟨10.1093/mnras/stv656⟩
Salumbides, E J, Bagdonaite, J, Abgrall, H, Roueff, E & Ubachs, W M G 2015, ' H-2 Lyman and Werner band lines and their sensitivity for a variation of the proton-electron mass ratio in the gravitational potential of white dwarfs ', Monthly Notices of the Royal Astronomical Society, vol. 450, no. 2, pp. 1237-1245 . https://doi.org/10.1093/mnras/stv656
Monthly Notices of the Royal Astronomical Society, 2015, 450 (2), pp.1237-1245. ⟨10.1093/mnras/stv656⟩
Recently we published an accurate analysis of molecular hydrogen absorption in the photospheres of the white dwarf stars GD133 and GD29-38, previously observed with the Cosmic Origins Spectrograph aboard the Hubble Space Telescope. Constraints were d
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 630, pp.A58. ⟨10.1051/0004-6361/201936249⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 630, pp.A58. ⟨10.1051/0004-6361/201936249⟩
The high spectral resolution R about 45,000 provided by IGRINS (Immersion Grating INfrared Spectrometer) at MacDonald Observatory and R 100,000 achieved by CRIRES (CRyogenic high-resolution InfraRed Echelle Spectrograph) at VLT (Very Large Telescope)
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Publikováno v:
Journal of Molecular Spectroscopy, 253(1), 64-72. Academic Press Inc.
Energies and probabilities of Lyman transitions of high rovibrationally excited H 2 , HD and D 2 molecules have been measured and compared with calculations. The experimental results are obtained from laser-induced fluorescence spectra that have been
Publikováno v:
The Astrophysical Journal Supplement Series. 177:388-407
At high resolving power -->(?/? ? ? 10,000) , we have measured the electron impact-induced fluorescence spectrum of H2 from 3300-10000 ? at 20 and 100 eV. We have analyzed the visible-optical-near-IR (VOIR) emission spectrum under optically thin, sin
Autor:
Evelyne Roueff, H. Abgrall
Publikováno v:
Astronomy & Astrophysics. 445:361-372
In this paper, we derive the theoretical properties of rovibrational levels belonging to excited B, C, B' , and D electronic states of HD. We compute the eigenvalues and eigenfunctions of the nuclear coupled Schroedinger equations using ab initio ele
Autor:
H. Abgrall, J. Gustin, Jean-Claude Gérard, Jean-Michel Desert, Paul D. Feldman, David J. Sahnow, Alfred Vidal-Madjar, J. H. Waite, Harold A. Weaver, Joseph M. Ajello, Denis Grodent, E. Roueff, H. W. Moos, L. Ben Jaffel, Brian C. Wolven
Publikováno v:
Icarus. 171:336-355
High-resolution ( ∼ 0.22 A ) spectra of the north jovian aurora were obtained in the 905–1180 A window with the Far Ultraviolet Spectroscopic Explorer (FUSE) on October 28, 2000. The FUSE instrument resolves the rotational structure of the H2 spe