Zobrazeno 1 - 10
of 23
pro vyhledávání: '"laboratory: solid state [methods]"'
Autor:
Harold Linnartz, D. M. Paardekooper, M. Bulak, C. Eistrup, Gleb Fedoseev, J. Terwisscha van Scheltinga, K.-J. Chuang
Publikováno v:
Astronomy & Astrophysics, 657:A120
Astron. Astrophys.
Astronomy and Astrophysics
Astron. Astrophys.
Astronomy and Astrophysics
Context. The Rosetta and Giotto missions investigated the composition of the cometary comae of 67P/Churyumov-Gerasimenko and 1P/Halley, respectively. In both cases, a surprisingly large amount of molecular oxygen (O2) was detected and was well correl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::289b69a2146e75f7f488a2647a4608d5
http://hdl.handle.net/1887/3514949
http://hdl.handle.net/1887/3514949
Autor:
C. Scirè, G. A. Baratta, Th. Henning, K.-J. Chuang, Cornelia Jäger, Maria Elisabetta Palumbo, Harold Linnartz, Gleb Fedoseev
Publikováno v:
Astronomy & Astrophysics, 650
Astron. Astrophys.
Astronomy and Astrophysics
Astron. Astrophys.
Astronomy and Astrophysics
The simultaneous detection of organic molecules of the form C$_2$H$_{\text{n}}$O, such as ketene (CH$_2$CO), acetaldehyde (CH$_3$CHO), and ethanol (CH$_3$CH$_2$OH), toward early star-forming regions offers hints of shared chemical history. Several re
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bd4d0c7ee549f03a7d7ab2461b003252
https://hdl.handle.net/1887/3250933
https://hdl.handle.net/1887/3250933
Publikováno v:
Astronomy & Astrophysics
Astron. Astrophys.
Astronomy and Astrophysics
Astronomy & Astrophysics, 647, 1-17
Astron. Astrophys.
Astronomy and Astrophysics
Astronomy & Astrophysics, 647, 1-17
Context. Many C-, O-, and H-containing complex organic molecules (COMs) have been observed in the interstellar medium (ISM) and their formation has been investigated in laboratory experiments. An increasing number of recent detections of large N-bear
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2020, 494 (2), pp.2396-2409. ⟨10.1093/mnras/staa778⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, 494 (2), pp.2396-2409. ⟨10.1093/mnras/staa778⟩
Rachid, M G, Pilling, S, Rocha, W R M, Agnihotri, A, Rothard, H & Boduch, P 2020, ' Processing of 72-K water-rich ices by keV and MeV oxygen ions : implications for the Saturnian moon Enceladus ', Monthly Notices of the Royal Astronomical Society, vol. 494, no. 2, pp. 2396-2409 . https://doi.org/10.1093/mnras/staa778
Monthly Notices of the Royal Astronomical Society, 2020, 494 (2), pp.2396-2409. ⟨10.1093/mnras/staa778⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, 494 (2), pp.2396-2409. ⟨10.1093/mnras/staa778⟩
Rachid, M G, Pilling, S, Rocha, W R M, Agnihotri, A, Rothard, H & Boduch, P 2020, ' Processing of 72-K water-rich ices by keV and MeV oxygen ions : implications for the Saturnian moon Enceladus ', Monthly Notices of the Royal Astronomical Society, vol. 494, no. 2, pp. 2396-2409 . https://doi.org/10.1093/mnras/staa778
The processing of H2O:CO2:CH4 (10:1:1) and H2O:CO2:CH4:NH3 (10:1:1:1) ices at 72 K by oxygen ions was studied in an attempt to simulate the physicochemical effects induced by energetic ions on the surface of Enceladus (or similar cold surfaces in the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4b2de1acc5cdece5d58bc9899c27cd69
https://hal.science/hal-03033453/document
https://hal.science/hal-03033453/document
Publikováno v:
Astron. Astrophys.
Astronomy and Astrophysics
Astronomy & Astrophysics, 653, 1-33
Astronomy and Astrophysics
Astronomy & Astrophysics, 653, 1-33
Context. In the near future, high spatial and spectral infrared (IR) data of star-forming regions obtained by the James Webb Space Telescope may reveal new solid-state features of various species, including more intriguing classes of chemical compoun
Autor:
C. Santonja, M. Domingo, Ramón Luna-Ferrándiz, C. Millán, Miguel Angel Satorre, R. Luna, Georgina Gisbert
Publikováno v:
RiuNet. Repositorio Institucional de la Universitat Politécnica de Valéncia
instname
instname
[EN] The desorption process of methanol in the hot cores of massive young stars is addressed in this work. The study of pure methanol ice and when it is mixed or layered with water allows a better understanding of the physical and chemical processes
Amorphous solid water (ASW) is found on icy dust grains in the interstellar medium (ISM), as well as on comets and other icy objects in the outer solar system. The optical properties of ASW are thus relevant for many astrophysical environments, but i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______101::0b2e0f2081a62aa05b2717ef90bfbd23
https://dspace.library.uu.nl/handle/1874/408343
https://dspace.library.uu.nl/handle/1874/408343
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
12 pags., 8 figs., 3 tabs.
The interaction of volatile species with carbonaceous interstellar dust analogues is of relevance in the chemistry and physics of dense clouds in the interstellar medium. Two deposits of hydrogenated amorphous carbon (
The interaction of volatile species with carbonaceous interstellar dust analogues is of relevance in the chemistry and physics of dense clouds in the interstellar medium. Two deposits of hydrogenated amorphous carbon (
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::357b88874192384e2af2a8b2d69f55e3
http://hdl.handle.net/10261/208383
http://hdl.handle.net/10261/208383
Publikováno v:
Astronomy and Astrophysics
Aims. In this paper we investigate the detectability of the molecular oxygen in icy dust grain mantles towards astronomical objects. Methods. We present a systematic set of experiments with O2-H2O ice mixtures designed to disentangle how the molecula
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9ba10e1325da4078c5de8b417e0b27d3
http://arxiv.org/abs/1810.10811
http://arxiv.org/abs/1810.10811