Zobrazeno 1 - 10
of 31
pro vyhledávání: '"Inma Dominguez"'
Autor:
Antoaneta Antonova, Maarten Baes, Andreas Burkert, Roger L. Davies, Inma Dominguez, Lex Kaper, Nick D. Kylafis, Sara Lucatello, Georges Meylan, Agata Różańska
Publikováno v:
Nature Astronomy. 6:765-765
We revise the theoretical initial mass-final luminosity relation for progenitors of type IIP and IIL supernovae. The effects of the major uncertainties, as those due to the treatment of convection, semiconvection, rotation, mass loss, nuclear reactio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bc178e10c2afe0007a234304ecb2405e
Autor:
Lluís Galbany, Inma Dominguez
Publikováno v:
The European Physical Journal Plus. 133
Bright and homogeneous, thermonuclear, or type Ia, supernovae (SNeIa) are our best extragalactic distance indicators. Since the 60s, SNeIa have been used as cosmological tools, initially, to estimate the current expansion rate of the Universe, the Hu
Autor:
M. E. Moreno-Raya, Vallery Stanishev, R. A. Marino, A. Mourao, R. García-Benito, F. F. Rosales-Ortega, Lluís Galbany, Angel R. Lopez-Sanchez, W. M. Wood-Vasey, Joseph P. Anderson, Inma Dominguez, Santiago González-Gaitán, S. Pedraz, Sebastián F. Sánchez, K. A. Ponder, Hanindyo Kuncarayakti, Mercedes Mollá, José M. Vílchez, Carles Badenes
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
CIÊNCIAVITAE
NASA Astrophysics Data System
instname
CIÊNCIAVITAE
NASA Astrophysics Data System
We present the PMAS/PPak Integral-field Supernova hosts COmpilation (PISCO), which comprises integral field spectroscopy (IFS) of 232 supernova (SN) host galaxies that hosted 272 SNe, observed over several semesters with the 3.5 m telescope at the Ca
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d0da615f0f59a9fb91c810a5013c1950
http://urn.kb.se/resolve?urn=urn:nbn:se:liu:diva-147113
http://urn.kb.se/resolve?urn=urn:nbn:se:liu:diva-147113
Autor:
Marcella Marconi, Jacco Th. van Loon, Amanda I. Karakas, Claus Leitherer, Marco Limongi, John C. Lattanzio, Jordi Isern, Inma Dominguez, Corinne Charbonnel, Giora Shaviv
Publikováno v:
Proceedings of the International Astronomical Union. 11:436-452
Commission 35 (C35), “Stellar Constitution”, consists of members of the International Astronomical Union whose research spans many aspects of theoretical and observational stellar physics and it is mainly focused on the comprehension of the prope
Publikováno v:
Physical review letters. 113(19)
We derive a strong bound on the axion-photon coupling $g_{a\gamma}$ from the analysis of a sample of 39 Galactic Globular Clusters. As recognized long ago, the R parameter, i.e. the number ratio of stars in horizontal over red giant branch of old ste
Publikováno v:
The Astrophysical Journal. 554:1159-1174
New stellar models with mass ranging between 4 and 8 Mo, Z=0 and Y=0.23 are presented. The models have been evolved from the pre Main Sequence up to the Asymptotic Giant Branch (AGB). At variance with previous claims, we find that these updated stell
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 306:L1-L7
We show that the inclusion of axion emission during stellar evolution introduces important changes into the evolutionary behaviour of AGB stars. The mass of the resulting C/O white dwarf is much lower than the equivalent obtained from standard evolut
Autor:
Carlos Abia, Oscar Straniero, Gino Tosti, Jordi Isern, Josep Colomé, Mauro Dolci, Inma Dominguez, Fabio Roncella, Maurizio Busso, Giuliano Nucciarelli
Publikováno v:
Proceedings of the International Astronomical Union. 2:702-704
The IRAIT (International Robotic Antarctic Infrared Telescope) project (Tosti et al. 2006) is based on a 80 cm aperture telescope to observe in the infrared range. It is due to start operations in spring 2008, several months after installation in Dom
Publikováno v:
The Astrophysical Journal. 472:783-788
The effect of stellar rotation on the late evolution of intermediate-mass stars has been explored, employing very simple numerical methods. At the epoch of central He exhaustion and C-O core formation, even an initially small rotation may induce, for