Zobrazeno 1 - 10
of 57
pro vyhledávání: '"ISM: cloud"'
Autor:
Ziwei Wu, William A Coles, Joris P W Verbiest, Krishnakumar Moochickal Ambalappat, Caterina Tiburzi, Jean-Mathias Grießmeier, Robert A Main, Yulan Liu, Michael Kramer, Olaf Wucknitz, Nataliya Porayko, Stefan Osłowski, Ann-Sofie Bak Nielsen, Julian Y Donner, Matthias Hoeft, Marcus Brüggen, Christian Vocks, Ralf-Jürgen Dettmar, Gilles Theureau, Maciej Serylak, Vladislav Kondratiev, James W McKee, Golam M Shaifullah, Ihor P Kravtsov, Vyacheslav V Zakharenko, Oleg Ulyanov, Olexandr O Konovalenko, Philippe Zarka, Baptiste Cecconi, Léon V E Koopmans, Stéphane Corbel
Publikováno v:
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2023, 520 (4), pp.5536-5543. ⟨10.1093/mnras/stad429⟩
Mon.Not.Roy.Astron.Soc., 2023, 520 (4), pp.5536-5543. ⟨10.1093/mnras/stad429⟩
Interstellar scattering (ISS) of radio pulsar emission can be used as a probe of the ionised interstellar medium (IISM) and causes corruptions in pulsar timing experiments. Two types of ISS phenomena (intensity scintillation and pulse broadening) are
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::83704b5ff24d4703ff540ef1e7746c8f
https://doi.org/10.1093/mnras/stad429
https://doi.org/10.1093/mnras/stad429
Autor:
Izaskun Jiménez-Serra, Lucas F. Rodríguez-Almeida, Jesús Martín-Pintado, Víctor M. Rivilla, Mattia Melosso, Shaoshan Zeng, Laura Colzi, Yoshiyuki Kawashima, Eizi Hirota, Cristina Puzzarini, Belén Tercero, Pablo de Vicente, Fernando Rico-Villas, Miguel A. Requena-Torres, Sergio Martín
Theories on the origins of life propose that early cell membranes were synthesized from amphiphilic molecules simpler than phospholipids such as fatty alcohols. The discovery in the interstellar medium (ISM) of ethanolamine, the simplest phospholipid
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::20c9ab5e13e6652b98a9e781674b5ea3
http://arxiv.org/abs/2204.08267
http://arxiv.org/abs/2204.08267
Autor:
F. Fontani, A. Schmiedeke, A. Sánchez-Monge, L. Colzi, D. Elia, V. M. Rivilla, M. T. Beltrán, L. Bizzocchi, P. Caselli, L. Magrini, D. Romano
Context. The outer Galaxy is an environment with a lower metallicity than the regions surrounding the Sun and for this reason the formation and survival of molecules in star-forming regions located in the inner and outer Galaxy are expected to be dif
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______4094::5808bf013bf90979ab2bd8deaac22e5b
https://hdl.handle.net/11585/900738
https://hdl.handle.net/11585/900738
Autor:
Fontani, F., Colzi, L., Bizzocchi, L., Rivilla, V. M., Elia, D., Beltrán, M. T., Caselli, P., Magrini, L., Sánchez-Monge, A., Testi, L., Romano, D.
The outer Galaxy is an environment with metallicity lower than the Solar one. Because of this, the formation and survival of molecules in star-forming regions located in the inner and outer Galaxy is expected to be different. To gain understanding on
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2b6cda0fd4938f33fea9983383a42449
Publikováno v:
Monthly Notices of the RAS (0035-8711), 487(3), 3377-3391
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society
We study the photoevaporation of Jeans-unstable molecular clumps by isotropic FUV (6 eV $< {\rm h}��$ < 13.6 eV) radiation, through 3D radiative transfer hydrodynamical simulations implementing a non-equilibrium chemical network that includes the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d1272d763cf0d4067930087b1cdbf0a8
https://doi.org/10.1093/mnras/stz1527
https://doi.org/10.1093/mnras/stz1527
Context. The nitrogen isotopic ratio is considered an important diagnostic tool of the star formation process, and $N_2H^+$ is particularly important because it is directly linked to molecular nitrogen $N_2$. However, theoretical models still lack to
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::978594dafd226b529eca42f61ad0e43b
http://arxiv.org/abs/2010.05954
http://arxiv.org/abs/2010.05954
Autor:
Stefano Pezzuto, Alberto Noriega-Crespo, Manuel Merello, David Eden, Giuseppe Riccio, Luca Olmi, Fabio Vitello, Nicolas Peretto, Sergio Molinari, Eva Sciacca, Eugenio Schisano, G. Li Causi, P. Palmeirim, Annie Zavagno, M. T. Beltrán, A. M. di Giorgio, M. Benedettini, Anthony Peter Whitworth, Toby J. T. Moore, Massimo Brescia, Davide Elia, Marco Molinaro, Leonardo Testi, Ugo Becciani, L. Cambresy, G. Umana, A. Baldeschi, S. J. Liu, Alessio Traficante, Stefano Cavuoti
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters
Monthly Notices of the Royal Astronomical Society: Letters, Oxford Journals, In press
Monthly Notices of the Royal Astronomical Society: Letters, Oxford Journals, In press, 492 (4), pp.5420-5455. ⟨10.1093/mnras/staz3466⟩
Monthly Notices of the Royal Astronomical Society: Letters, In press, 492 (4), pp.5420-5455. ⟨10.1093/mnras/staz3466⟩
Monthly Notices of the Royal Astronomical Society: Letters, Oxford Journals, In press
Monthly Notices of the Royal Astronomical Society: Letters, Oxford Journals, In press, 492 (4), pp.5420-5455. ⟨10.1093/mnras/staz3466⟩
Monthly Notices of the Royal Astronomical Society: Letters, In press, 492 (4), pp.5420-5455. ⟨10.1093/mnras/staz3466⟩
The recent data collected by {\it Herschel} have confirmed that interstellar structures with filamentary shape are ubiquitously present in the Milky Way. Filaments are thought to be formed by several physical mechanisms acting from the large Galactic
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::db36e037d9ee0e453f06de3ecae15b2e
https://orca.cardiff.ac.uk/id/eprint/127618/1/1912.04020am.pdf
https://orca.cardiff.ac.uk/id/eprint/127618/1/1912.04020am.pdf
Autor:
Sergio Martín, Jesús Martín-Pintado, Jean-Claude Guillemin, Victor M. Rivilla, Barbara M. Giuliano, Luca Bizzocchi, Shaoshan Zeng, Andrea Pietropolli-Charmet, Paola Caselli, D. Prudenzano, M. A. Requena-Torres, Fernando Rico-Villas, Izaskun Jiménez-Serra
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 640, ⟨10.1051/0004-6361/202038083⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Astronomy & Astrophysics
Astronomy and Astrophysics-A&A, 2020, 640, ⟨10.1051/0004-6361/202038083⟩
Instituto Nacional de Técnica Aeroespacial (INTA)
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 640, ⟨10.1051/0004-6361/202038083⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Astronomy & Astrophysics
Astronomy and Astrophysics-A&A, 2020, 640, ⟨10.1051/0004-6361/202038083⟩
Instituto Nacional de Técnica Aeroespacial (INTA)
Context. Small imines containing up to three carbon atoms are present in the interstellar medium (ISM). As alkynyl compounds are abundant in this medium, propargylimine (2-propyn-1-imine, HC C-CH =NH) thus represents a promising candidate for a new i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5f09ca3f5011d99ee14157fd13fc42d9
https://hdl.handle.net/11585/872452
https://hdl.handle.net/11585/872452
Autor:
Fabio Reale, David N. Burrows, Kari A. Frank, Giovanni Peres, Oleh Petruk, Salvatore Orlando, Fabrizio Bocchino, Costanza Argiroffi, Marco Miceli
Astrophysical shocks at all scales, from those in the heliosphere up to the cosmological shock waves, are typically "collisionless", because the thickness of their jump region is much shorter than the collisional mean free path. Across these jumps, e
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5de66afc8104edd56d0b243ec9f853f7
http://hdl.handle.net/10447/339488
http://hdl.handle.net/10447/339488
Autor:
A. Vasyunin, Barbara M. Giuliano, Ana Chacón-Tanarro, Paola Caselli, Anna Punanova, Luca Bizzocchi, Jaime E. Pineda, Valerio Lattanzi, Silvia Spezzano, Olli Sipilä
Publikováno v:
Astronomy and Astrophysics
The study of deuteration in pre-stellar cores is important to understand the physical and chemical initial conditions in the process of star formation. In particular, observations toward pre-stellar cores of methanol and deuterated methanol, solely f
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ca43439cc52753c45e3c8ee565b3c017
https://elar.urfu.ru/handle/10995/90537
https://elar.urfu.ru/handle/10995/90537