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Repositorios
68
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Ciencias Astronómicas
Física
8
Galaxies: evolution
7
Galaxies: star clusters
7
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5
Methods: numerical
5
White dwarfs
5
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4
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4
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4
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4
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4
Astrophysics
3
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3
Cosmology: theory
3
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3
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3
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3
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3
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3
H ii regions
3
ISM: abundances
3
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Astronomy
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Ciencias Exactas
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Dense matter
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Galaxies: abundances
2
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1por Awan, Humna, Gawiser, Eric, Kurczynski, Peter, Jones, R. Lynne, Zhan, Hu, Padilla, Nelson D., Muñoz Arancibia, Alejandra M., Orsi, Álvaro, Cora, Sofía Alejandra, Yoachim, Peter“... on different timescales (per season, per night, per visit). Our results illustrate that per night and per visit...”
Publicado 2016
Aportado por: SEDICI (UNLP)Articulo -
2“... of these harmonics or sidebands, with 95 per cent confidence upper limits to their power between ∼1 and ∼10 per cent...”
Aportado por: SEDICI (UNLP)Articulo -
3“... of the order of a Hubble time, even though they had very large fractions of chaotic orbits (more than 85 per...”
Aportado por: SEDICI (UNLP)Articulo -
4por Brunini, Adrián“... shorter than the one of single Centaurs. Nearly 10 per cent of the binaries reach a very tight circular...”
Publicado 2014
Aportado por: SEDICI (UNLP)Articulo -
5“... produced Wolf–Rayet binary frequency to be 52±14 per cent in the Large Magellanic Cloud and 100 per cent...”
Aportado por: SEDICI (UNLP)Articulo -
6por Perez, María Josefa, Tissera, Patricia Beatriz, Padilla, N., Alonso, M. S., Lambas, D. G.“... in the red fraction between close pairs and the control galaxies increases from ∼10 per cent in low-mass...”
Publicado 2009
Aportado por: SEDICI (UNLP)Articulo -
7por Tecce, Tomás E., Cora, Sofía Alejandra, Tissera, Patricia B., Abadi, Mario G., Lagos, Claudia del Pilar“...>vir</SUB>≃ 10<SUP>15</SUP> h<SUP>-1</SUP> M⊙, over 50 per cent of satellite galaxies have experienced...”
Publicado 2010
Aportado por: SEDICI (UNLP)Articulo -
8“... of the SMC about the LMC.We find that, for orbital eccentricities e ≥ 0.4, approximately 15 per cent...”
Aportado por: SEDICI (UNLP)Articulo -
9“... to about 40 per cent of its mass from the galaxy where it belongs. Nevertheless, in those experiments...”
Aportado por: SEDICI (UNLP)Articulo -
10“...-dimensional vectors per season that include wind direction frequencies, calms and mean wind speeds per wind...”
Aportado por: SEDICI (UNLP)Articulo -
11“... than 3 per cent over one Hubble time and, moreover, we show that the most likely cause of those changes...”
Aportado por: SEDICI (UNLP)Articulo -
12por Romero, Alejandra D., Kepler, S. O., Joyce, S. R. G., Lauffer, G. R., Córsico, Alejandro Hugo“... in the radius of the model of up to ∼12 per cent. This translates directly to an increase in log g for a fixed...”
Publicado 2019
Aportado por: SEDICI (UNLP)Articulo -
13“... of the diffuse stellar populations in early-type galaxies if the number of clusters per unit stellar mass depends...”
Aportado por: SEDICI (UNLP)Articulo -
14por Torres, Santiago, Rebassa Mansergas, Alberto, Camisassa, María Eugenia, Raddi, Roberto“... Gyr. The mass distribution of the sample peaks at 0.589M⊙, with 71 per cent of the white dwarf masses...”
Publicado 2021
Aportado por: SEDICI (UNLP)Articulo Preprint -
15“...We have examined the interstellar medium in the vicinity of massive stars belonging to the Per OB1...”
Aportado por: SEDICI (UNLP)Articulo -
16“... of field contact binaries. V53 is a high mass-ratio (q = 1.230 ± 0.004), deep-contact (f = 79.7 ± 1.9 per...”
Aportado por: SEDICI (UNLP)Articulo -
17por Mancuso, Giulio Cesare“... at 9.6 ± 0.5 mHz with a fractional rms amplitude of 2.2 ± 0.2 per cent (0.5–10 keV), likely due...”
Publicado 2020
Aportado por: SEDICI (UNLP)Articulo -
18por Scóccola, Claudia Graciela“... accuracy (1 per cent level) at small scales, i.e. r < 25 h<SUP>-1</SUP> Mpc or k > 0.15 h Mpc<SUP>-1</SUP...”
Publicado 2015
Aportado por: SEDICI (UNLP)Articulo -
19por Olano, Carlos Alberto“... increment of 100 per cent and a cloud's velocity variation of 30 km s<SUP>-1</SUP>, from the beginning...”
Publicado 2015
Aportado por: SEDICI (UNLP)Articulo -
20por Löbling, L., Rauch, Thomas, Miller Bertolami, Marcelo Miguel, Todt, Helge, Friederich, Felix, Ziegler, M., Werner, Klaus, Kruk, Jeffrey W.“... to stellar evolution models the result is a star with a surface composition of H≈20 per cent by mass (AFTP...”
Publicado 2019
Aportado por: SEDICI (UNLP)Articulo