Zobrazeno 1 - 10
of 32
pro vyhledávání: '"C Badenes"'
Autor:
T Jayasinghe, Todd A Thompson, C S Kochanek, K Z Stanek, D M Rowan, D V Martin, Kareem El-Badry, P J Vallely, J T Hinkle, D Huber, H Isaacson, J Tayar, K Auchettl, I Ilyin, A W Howard, C Badenes
We report the discovery of a stripped giant + lower giant binary, 2M04123153+6738486 (2M0412), identified during a search for non-interacting compact object-star binaries. 2M0412 is an evolved ($T_{\rm eff, giant}\simeq4000$ K), luminous ($L_{\rm gia
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cb276c2ab3b0ec5610e83c3f84ec8c5d
http://arxiv.org/abs/2201.11131
http://arxiv.org/abs/2201.11131
Autor:
José María Bellón, María José Calvo-Alcántara, Juana Benedí, A Mataix‐Sanjuan, J. C. López, Leire Pérez-Latorre, Beatriz López-Centeno, Saye Khoo, Juan Berenguer, Catia Marzolini, C Badenes‐Olmedo
Publikováno v:
HIV MEDICINE
Objectives We assessed the prevalence of potentially inappropriate medication (PIM) among older (≥ 65 years) people living with HIV (O-PLWH) in the region of Madrid. Methods We analysed the dispensation registry of community and hospital pharmacies
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::dec8217868409cae718f46582d9a2b0e
Publikováno v:
Nature Astronomy. 1:800-804
Type Ia supernovae have proven vital to our understanding of cosmology, both as standard candles and for their role in galactic chemical evolution; however, their origin remains uncertain. The canonical accretion model implies a hot and luminous prog
Autor:
C. Badenes, Franz E. Bauer, J. Quirola-Vasquez, T. Nymark, Dom Walton, Vikram V. Dwarkadas, W. N. Brandt
Publikováno v:
Mon Not R Astron Soc
We present X-ray spectra spanning 18 years of evolution for SN\,1996cr, one of the five nearest SNe detected in the modern era. {\it Chandra} HETG exposures in 2000, 2004, and 2009 allow us to resolve spectrally the velocity profiles of Ne, Mg, Si, S
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4618216bd2c0b99bae2495f9a26460e3
http://arxiv.org/abs/1910.03710
http://arxiv.org/abs/1910.03710
Autor:
Alberto D. Bolatto, Leo Blitz, Helmut Dannerbauer, Lluís Galbany, C. Badenes, Tony Wong, Dyas Utomo, Santiago González-Gaitán, G. van de Ven, Miguel A. Pérez-Torres, Keiichi Maeda, Sebastian Perez, Sebastián F. Sánchez, L. Mora, Raffaella Anna Marino, Angel R. Lopez-Sanchez
Publikováno v:
NASA Astrophysics Data System
CIÊNCIAVITAE
CIÊNCIAVITAE
CO observations allow estimations of the gas content of molecular clouds, which trace the reservoir of cold gas fuelling star formation, as well as to determine extinction via H$_2$ column density, N(H$_2$). Here, we studied millimetric and optical p
The evolutionary mechanism underlying Type Ia supernova explosions remains unknown. Recent efforts to constrain progenitor models based on the influence that their high energy emission would have on the interstellar medium (ISM) of galaxies have prov
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fc4d7370f26616443c4748aae7c408ad
Autor:
C. Badenes
Publikováno v:
Proceedings of the National Academy of Sciences. 107:7141-7146
The unprecedented spatial and spectral resolutions of Chandra have revolutionized our view of the X-ray emission from supernova remnants. The excellent data sets accumulated on young, ejecta dominated objects like Cas A or Tycho present a unique oppo
Autor:
Jürgen Knödlseder, G. Vedrenne, Rashid Sunyaev, G. G. Lichti, Simona Soldi, A. Domingo, Matthieu Renaud, P. von Ballmoos, Jordi Isern, E. M. Churazov, Inmaculada Domínguez, F. Lebrun, P. Hoeflich, C. Badenes, Domingo García-Senz, P. Jean, Nancy Elias-Rosa, Margarita Hernanz, Eduardo Bravo, Dieter H. Hartmann
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2016, 588, pp.A67. ⟨10.1051/0004-6361/201526941⟩
Astron.Astrophys.
Astron.Astrophys., 2016, 588, pp.A67. ⟨10.1051/0004-6361/201526941⟩
Recercat. Dipósit de la Recerca de Catalunya
instname
Astronomy and Astrophysics-A&A, 2016, 588, pp.A67. ⟨10.1051/0004-6361/201526941⟩
UPCommons. Portal del coneixement obert de la UPC
Universitat Politècnica de Catalunya (UPC)
Astron.Astrophys., 2016, 588, pp.A67. 〈10.1051/0004-6361/201526941〉
Astronomy and Astrophysics-A&A, EDP Sciences, 2016, 588, pp.A67. ⟨10.1051/0004-6361/201526941⟩
Astron.Astrophys.
Astron.Astrophys., 2016, 588, pp.A67. ⟨10.1051/0004-6361/201526941⟩
Recercat. Dipósit de la Recerca de Catalunya
instname
Astronomy and Astrophysics-A&A, 2016, 588, pp.A67. ⟨10.1051/0004-6361/201526941⟩
UPCommons. Portal del coneixement obert de la UPC
Universitat Politècnica de Catalunya (UPC)
Astron.Astrophys., 2016, 588, pp.A67. 〈10.1051/0004-6361/201526941〉
Context. The optical light curve of Type Ia supernovae (SNIa) is powered by thermalized gamma-rays produced by the decay of 56Ni and 56Co, the main radioactive isotopes synthesized by the thermonuclear explosion of a C/O white dwarf. Aims: Gamma-rays
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3a0ac3aae5b8d98ed9dc22d144863f5e
https://hal.archives-ouvertes.fr/hal-01554942
https://hal.archives-ouvertes.fr/hal-01554942
Autor:
Damian Mast, A. Mourao, José M. Vílchez, C. Kehrig, C. Badenes, Rubén García-Benito, G. van de Ven, C. J. Walcher, Sebastián F. Sánchez, Lluís Galbany, Mercedes Mollá, Myriam Rodrigues, Vallery Stanishev, Sharon E. Meidt, Hector Flores, Mariya Lyubenova, R. M. González Delgado, Enrique Pérez, Raffaella Anna Marino
Publikováno v:
Astronomy and astrophysics, 591(July 2016):A48. EDP Sciences
Digital.CSIC. Repositorio Institucional del CSIC
instname
CIÊNCIAVITAE
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
ASTRONOMY & ASTROPHYSICS
NASA Astrophysics Data System
E-Prints Complutense. Archivo Institucional de la UCM
Digital.CSIC. Repositorio Institucional del CSIC
instname
CIÊNCIAVITAE
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
ASTRONOMY & ASTROPHYSICS
NASA Astrophysics Data System
E-Prints Complutense. Archivo Institucional de la UCM
The metallicity of a supernova progenitor, together with its mass, is one of the main parameters that can rule the progenitor's fate. We present the second study of nearby supernova (SN) host galaxies (0.005 10 dex) by targeted searches. We neither f
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c2d038d009befd372cdd0ed86a1511df
https://research.rug.nl/en/publications/113f611b-ccf8-45ad-9858-ab7b23621ccc
https://research.rug.nl/en/publications/113f611b-ccf8-45ad-9858-ab7b23621ccc
Autor:
N. Prasert, D. Koester, J. J. Hermes, Avishay Gal-Yam, S. Kengkriangkrai, Madelon C. P. Bours, S. E. Thompson, Boris T. Gänsicke, Alina G. Istrate, M. Kilic, C. Badenes, John R. Thorstensen, Thomas M. Tauris, V. S. Dhillon, T. R. Marsh, F. Mullally, D. Steeghs
We present Hubble Space Telescope UV spectra of the 4.6 h period double white dwarf SDSS J125733.63+542850.5. Combined with Sloan Digital Sky Survey optical data, these reveal that the massive white dwarf (secondary) has an effective temperature T2 =
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::aa80370ff779f17f9c8ccb97f484b2e4
https://eprints.whiterose.ac.uk/122718/1/stv889.pdf
https://eprints.whiterose.ac.uk/122718/1/stv889.pdf