Zobrazeno 1 - 8
of 8
pro vyhledávání: '"E M, Penteado"'
Molecules in space are synthesized via a large variety of gas-phase reactions, and reactions on dust-grain surfaces, where the surface acts as a catalyst. Especially, saturated, hydrogen-rich molecules are formed through surface chemistry. Astrochemi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5eb33e13c9abfd4cfc959ac63002f76e
Publikováno v:
Monthly notices of the Royal Astronomical Society. 454(1)
The prominent infrared absorption band of solid CO - commonly observed towards young stellar objects (YSOs) - consists of three empirically determined components. The broad 'red component' (2136 cm
Publikováno v:
The Astrophysical Journal, 844, 1-13
The Astrophysical Journal, 844, 1, pp. 1-13
ASTROPHYSICAL JOURNAL (ISSN 0004-637X), 844(1), 71
The Astrophysical Journal, 844, 1, pp. 1-13
ASTROPHYSICAL JOURNAL (ISSN 0004-637X), 844(1), 71
Advanced telescopes, such as ALMA and JWST, are likely to show that the chemical universe may be even more complex than currently observed, requiring astrochemical modelers to improve their models to account for the impact of new data. However, essen
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5ee946c915800d8e769ed3f9a4451426
https://hdl.handle.net/1887/59275
https://hdl.handle.net/1887/59275
Autor:
Thanja Lamberts, Robin T. Garrod, E. M. Penteado, D. Semenov, Catherine Walsh, Sergio Ioppolo, Herma M. Cuppen
Publikováno v:
Space Science Reviews
Space Science Reviews, 212, 1-58
Space Science Reviews, 212(1-2), 1-58
Space Science Reviews, 212, 1, pp. 1-58
Space Science Reviews, 212, 1-58
Space Science Reviews, 212(1-2), 1-58
Space Science Reviews, 212, 1, pp. 1-58
The cross-disciplinary field of astrochemistry exists to understand the formation, destruction, and survival of molecules in astrophysical environments. Molecules in space are synthesized via a large variety of gas-phase reactions, and reactions on d
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ced69ae8d8f0de18271f36f42e6afce5
https://doi.org/10.1007/s11214-016-0319-3
https://doi.org/10.1007/s11214-016-0319-3
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 439, 3616-3629
Monthly Notices of the Royal Astronomical Society, 439, 4, pp. 3616-3629
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 439, 4, pp. 3616-3629
Monthly Notices of the Royal Astronomical Society
The Galaxy is in continuous elemental evolution. Since new elements produced by dying stars are delivered to the interstellar medium, the formation of new enerations of stars and planetary systems is influenced by this metal enrichment. We aim to stu
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 417:2809-2816
With this paper we provide a solution to a disagreement between astronomical- and laboratorybased CO-ice spectroscopic data. In observations towards icy sources, the CO-ice stretching band comprises a prominent and broad ‘red component’ around 21
Spectroscopic constraints on CH3OH formation: CO mixed with CH3OH ices towards young stellar objects
Autor:
Klaus M. Pontoppidan, Adwin Boogert, Geoffrey A. Blake, E. M. Penteado, Herma M. Cuppen, Sergio Ioppolo
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 454, 1, pp. 531-540
Monthly Notices of the Royal Astronomical Society, 454, 531-540
Monthly Notices of the Royal Astronomical Society, 454, 531-540
The prominent infrared absorption band of solid CO – commonly observed towards young stellar objects (YSOs) – consists of three empirically determined components. The broad ‘red component’ (2136 cm^(−1), 4.681 μm) is generally attributed t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1311e516cb4ee6c2f343f02f12acf21f
https://hdl.handle.net/2066/149321
https://hdl.handle.net/2066/149321
Publikováno v:
Astrophysical Journal; 7/20/2017, Vol. 844 Issue 1, p1-1, 1p