Zobrazeno 1 - 10
of 168
pro vyhledávání: '"Iron peak"'
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 506:2725-2738
Quasar Q0059–2735, one of the first known iron low-ionization broad-absorption-line quasars (FeLoBAL), has a plethora of outflow absorption features at different velocities. Given multiple outflow systems, their troughs from high-ionization transit
Autor:
Swetlana Hubrig, Silva P. Järvinen, H. Adigozalzade, Ilya Ilyin, Viktor Khalack, Gautier Mathys
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 499:2734-2743
High resolution spectropolarimetric observations of the strongly magnetic, super-slowly rotating rapidly oscillating Ap star HD166473 are used to investigate the implications of the presence of a variable strong magnetic field on the vertical and sur
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
Aims. The aim of this work is to determine fundamental parameters of three Ap stars, GO And (HD 4778), κ Psc (HD 220825), and 84 UMa (HD 120198), using spectroscopic techniques. By analysing these stars, we complete the sample of Ap stars for which
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::88f4e7f21047bc7a0c54911b33731757
http://hdl.handle.net/10261/260455
http://hdl.handle.net/10261/260455
The OCCASO survey (Open Clusters Chemical Abundances from Spanish Observatories) targets old OCs, observing in median 6 red clump stars in each of them. We use higher resolution spectroscopy (R > 65,000), high signal-to-noise (SNR~70), and wider wave
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6a5d46a61f4de2971c41a1d500c88a6c
Autor:
M. Van der Swaelmen, Loredana Prisinzano, Sergey E. Koposov, Gerard Gilmore, F. M. Jiménez-Esteban, A. Hourihane, Gražina Tautvaišienė, V. Adibekyan, M. Tsantaki, Elisa Delgado-Mena, Angela Bragaglia, R. D. Jeffries, Sofia Randich, S. G. Sousa, Rodolfo Smiljanic, Sarah L. Martell, Veronica Roccatagliata, Laura Magrini, G. Carraro, Valentina D'Orazi, M. Baratella, L. Morbidelli, Simone Zaggia, Paula Jofre, Jack Lewis, Lorenzo Spina, Luca Sbordone, Amelia Bayo, Silvano Desidera, Ulrike Heiter, G. G. Sacco, E. Franciosini, Clare Worley, Anais Gonneau, Emilio J. Alfaro, Thomas Bensby
Publikováno v:
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
instname
Digital.CSIC. Repositorio Institucional del CSIC
Instituto Nacional de Técnica Aeroespacial (INTA)
Baratella, M, D'Orazi, V, Carraro, G, Desidera, S, Randich, S, Magrini, L, Adibekyan, V, Smiljanic, R, Spina, L, Tsantaki, M, Tautvaisiene, G, Sousa, S G, Jofré, P, Jiménes-Esteban, F M, Delgado-Mena, E, Martell, S, Swaelmen, M V D, Roccatagliata, V, Gilmore, G, Alfaro, E J, Bayo, A, Bensby, T, Bragaglia, A, Franciosini, E, Gonneau, A, Heiter, U, Hourihane, A, Jeffries, R D, Koposov, S E, Morbidelli, L, Prisinzano, L, Sacco, G, Sbordone, L, Worley, C, Zaggia, S & Lewis, J 2020, ' The Gaia-ESO Survey: a new approach to chemically characterising young open clusters : I. Stellar parameters, and iron-peak, α-, and proton-capture elements★,★★ ', Astronomy and Astrophysics . https://doi.org/10.1051/0004-6361/201937055
instname
Digital.CSIC. Repositorio Institucional del CSIC
Instituto Nacional de Técnica Aeroespacial (INTA)
Baratella, M, D'Orazi, V, Carraro, G, Desidera, S, Randich, S, Magrini, L, Adibekyan, V, Smiljanic, R, Spina, L, Tsantaki, M, Tautvaisiene, G, Sousa, S G, Jofré, P, Jiménes-Esteban, F M, Delgado-Mena, E, Martell, S, Swaelmen, M V D, Roccatagliata, V, Gilmore, G, Alfaro, E J, Bayo, A, Bensby, T, Bragaglia, A, Franciosini, E, Gonneau, A, Heiter, U, Hourihane, A, Jeffries, R D, Koposov, S E, Morbidelli, L, Prisinzano, L, Sacco, G, Sbordone, L, Worley, C, Zaggia, S & Lewis, J 2020, ' The Gaia-ESO Survey: a new approach to chemically characterising young open clusters : I. Stellar parameters, and iron-peak, α-, and proton-capture elements★,★★ ', Astronomy and Astrophysics . https://doi.org/10.1051/0004-6361/201937055
Context. Open clusters are recognised as excellent tracers of Galactic thin-disc properties. At variance with intermediate-age and old open clusters, for which a significant number of studies is now available, clusters younger than ≲ 150 Myr have b
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::17b6ca5d8b17e39c28dfc12a42f8d96d
https://hdl.handle.net/20.500.12666/312
https://hdl.handle.net/20.500.12666/312
Autor:
Stefano Ettori, Ang Liu, Sabrina De Grandi, Fabio Gastaldello, Piero Rosati, Paolo Tozzi, Colin Norman
We study the chemical evolution of galaxy clusters by measuring the iron mass in the ICM after dissecting the abundance profiles into different components. We use Chandra archival observations of 186 morphologically regular clusters in the redshift r
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2c4e3a9548f2fc07fa677abede1dc8a2
http://hdl.handle.net/20.500.12386/31215
http://hdl.handle.net/20.500.12386/31215
Autor:
Ian U. Roederer, Christopher Sneden, John J. Cowan, Ann Merchant Boesgaard, Elizabeth A. Den Hartog, James E. Lawler, Jennifer Sobeck
We have obtained new detailed abundances of the Fe-group elements Sc through Zn (Z=21-30) in three very metal-poor ([Fe/H] $\approx -3$) stars: BD 03 740, BD -13 3442 and CD -33 1173. High-resolution ultraviolet HST/STIS spectra in the wavelength ran
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9ba4488099e9ff13f2a18c12e899963c
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:
Florian Lach, Friedrich K. Roepke, Benoit Côté, Ivo R. Seitenzahl, Ashley J. Ruiter, Sabrina Gronow
Publikováno v:
Astronomy & Astrophysics
We analyze the nucleosynthesis yields of various Type Ia supernova explosion simulations including pure detonations in sub- Chandrasekhar mass white dwarfs, double detonations and pure helium detonations of sub-Chandrasekhar mass white dwarfs with an
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::99d2007d7e1280178cb17c4395198356
Chemical abundance analysis of 13 southern symbiotic giants from high-resolution spectra at ∼1.56 μm
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 466:2194-2201
Symbiotic stars (SySt) are binaries composed of a star in the later stages of evolution and a stellar remnant. The enhanced mass-loss from the giant drives interacting mass exchange and makes these systems laboratories for understanding binary evolut