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Autor:
Pisani G. B., Ruffini R., Aimuratov Y., Bianco C. L., Karlica M., Kovacevic M., Moradi R., Muccino M., Penacchioni A. V., Primorac D., Rueda J. A., Wang Y.
Publikováno v:
EPJ Web of Conferences, Vol 168, p 04002 (2018)
In a series of recent publications, scientists from ICRANet, led by professor Remo Ruffini, have reached a novel comprehensive picture of gamma-ray bursts (GRBs) thanks to their development of a series of new theoretical approaches. Among those, the
Externí odkaz:
https://doaj.org/article/23476396d400435789c97db07bf3aab5
Publikováno v:
EPJ Web of Conferences, Vol 252, p 05004 (2021)
The knowledge of the equation of state is a key ingredient for many dynamical phenomena that depend sensitively on the hot and dense nuclear matter, such as the formation of protoneutron stars and hot neutron stars. In order to accurately describe th
Autor:
K. F. Schuster, Peter A. R. Ade, Guilaine Lagache, Martino Calvo, Ph. André, V. Revéret, A. Andrianasolo, Alessandro Monfardini, Florian Kéruzoré, R. Zylka, F. Mayet, Alexandre Beelen, Nicolas Peretto, R. Adam, O. Bourrion, J. F. Macías-Pérez, Simon Doyle, Carsten Kramer, Giampaolo Pisano, Charles Romero, Shibo Shu, L. Perotto, Florian Ruppin, Aurore Bacmann, F.-X. Désert, Ana Gómez, Nicolas Ponthieu, M. De Petris, J.-F. Lestrade, A. Ritacco, Johannes Goupy, Alain Benoit, A. Catalano, Herve Aussel, Bilal Ladjelate, Philip Daniel Mauskopf, E. F. C. Driessen, Helene Roussel, I. Ristorcelli, Andrew Rigby, Barbara Comis, Carole Tucker, Samuel Leclercq, A. Sievers, Aurelien Bideaud, Frédérique Motte
Publikováno v:
EPJ Web Conf.
mm Universe @ NIKA2
mm Universe @ NIKA2, Jun 2019, Grenoble, France. pp.00018, ⟨10.1051/epjconf/202022800018⟩
EPJ Web of Conferences, Vol 228, p 00018 (2020)
mm Universe @ NIKA2
mm Universe @ NIKA2, Jun 2019, Grenoble, France. pp.00018, ⟨10.1051/epjconf/202022800018⟩
EPJ Web of Conferences, Vol 228, p 00018 (2020)
Understanding where and when the mass of stars is determined is one of the fundamental, mostly unsolved, questions in astronomy. Here, we present the first results of GASTON, the Galactic Star Formation with NIKA2 large programme on the IRAM 30m tele
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::adf7a8fd8acc2fe1322e942c18fa6736
https://orca.cardiff.ac.uk/id/eprint/130292/1/epjconf_mmuniverse2019_00018.pdf
https://orca.cardiff.ac.uk/id/eprint/130292/1/epjconf_mmuniverse2019_00018.pdf
Autor:
Eugene Semenko
Publikováno v:
EPJ Web of Conferences, Vol 240, p 05003 (2020)
A strong and stable magnetic field covering the whole surface is a landmark of chemically peculiar or CP stars. To explain the origin of mag- netic stars, several hypotheses were proposed, which depending on the mech- anism and time of formation can
Autor:
P. Tuan-Anh, T T Thai, Pierre Darriulat, N. T. Phuong, Do Thi Hoai, Pham Ngoc Diep, Pham Tuyet Nhung
Publikováno v:
EPJ Web of Conferences, Vol 240, p 05001 (2020)
Millimetre ALMA observations of the nascent winds of several Oxygen rich AGB stars have revealed the high Doppler velocity wings in their spectra. However, the physics underlying their production is unclear. In this paper, we illustrate the argument
Autor:
G. Manicò, G. D’Agata, G. L. Guardo, N. de Séréville, C. Spitaleri, S. Romano, D. Lattuada, M. Lattuada, A. A. Oliva, Fairouz Hammache, Roberta Spartà, M. La Commara, M. L. Sergi, A. Tumino, Maria Letizia Pumo, S. Palmerini, M. Mazzocco, G. G. Rapisarda, I. Indelicato, S. Cherubini, S. Messina, S. Hayakawa, M. La Cognata, M. Gulino, P. Figuera, A. Cvetinović, Neven Soić, A. Di Pietro, R. G. Pizzone, L. Lamia
Publikováno v:
EPJ Web of Conferences, Vol 227, p 02007 (2020)
EPJ Web Conf.
EPJ Web Conf.
Neutron induced reactions are fundamental for the nucleosynthesis of elements in the universe. Indeed, to correctly study the reactions involved in the well-known s-process in stars, which produce about half of the elements beyond the iron peak, it i
Autor:
Mounib F. El Eid, Cynthia Saad
Publikováno v:
EPJ Web of Conferences, Vol 227, p 01005 (2020)
The first stars have transformed the universe from the infrared background to the light. Thereby, this so called “dark age” ended by re-ionization through the ultraviolet light of the first stars. A short overview is given about the cosmological
Publikováno v:
EPJ Web of Conferences, Vol 240, p 05002 (2020)
We present a brief review of the recent results of photometric and spectroscopic surveys and 3-D hydrodynamic simulations of the mass- transfer for the class of oscillating mass-accreting components of Algols (oEA stars). These ground-based spectrosc
Autor:
Xiwen Qiang
Publikováno v:
EPJ Web of Conferences, Vol 237, p 06014 (2020)
Ranged-resolved profiles of atmospheric turbulence are necessary and important for many applications in astronomical and adaptive optics communities. In order to characterize the vertical atmospheric structure in field, a technique is put forward to
Publikováno v:
EPJ Web of Conferences, Vol 240, p 07012 (2020)
Stellar streams are stars which are trapped in the same potensial caused by dynamical resonance or tidal force. We aim to analyze kinematic sub- structures (streams) in the Galactic halo by V vs √ U2+ 2V 2 planes of Arifyanto & Fuchs. We crossmatch