Zobrazeno 1 - 10
of 272
pro vyhledávání: '"M, Galliano"'
Autor:
Bruce B Duncan, Maria Inês Schmidt, Paula A Bracco, Maria A Nunes, Kadhija A Cherubini, Cristina D Castilhos, Jainara Z Spagiari, Leony M Galliano, Ruben Ladwig, Fabricio B Del Vecchio, Anelita H M Del Vecchio, Michele Drehmer, Adriana Costa Forti, Cristina Façanha, Lenita Zajdenverg, Bianca de Almeida-Pititto, Rosângela Roginski Réa, Patrícia Medici Dualib
Publikováno v:
BMJ Open, Vol 14, Iss 10 (2024)
Objectives To evaluate a postpartum telephone-based lifestyle intervention to prevent diabetes in high-risk women with recent gestational diabetes mellitus (GDM).Design Multicentre parallel randomised clinical trial.Setting Specialised antenatal clin
Externí odkaz:
https://doaj.org/article/38bf2c35d3764c4e80c95f779440d9e6
Autor:
Gustavo Z. Schaun, Cristine L. Alberton, Maria Laura Brizio Gomes, Graciele F. Mendes, Mariana S. Häfele, Luana S. Andrade, Paula C. Campelo, Hector K. Ferreira, Lorena L. Oppelt, Leony M. Galliano, Leonardo Alves, Vinícius A. de Ataides, Marco A. Carmona, Rafael Lázaro, Stephanie S. Pinto, Eurico N. Wilhelm
Publikováno v:
Journal of Sports Sciences. 40:1399-1405
The present study aimed to investigate whether training status would influence the capacity of a verification phase (VER) to confirm maximal oxygen uptake (VO2max) of a previous graded exercise test (GXT) in individuals with hypertension. Twelve olde
Publikováno v:
Medicine & Science in Sports & Exercise. 54:321-321
Aims. The purpose of this work is the characterization of the main scaling relations between all of the interstellar medium (ISM) components, namely dust, atomic, molecular, and total gas, and gas-phase metallicity, as well as other galaxy properties
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2127::88669bbe03cb7b4c7e0111c64df627a3
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3068812
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3068812
Context. Dust in late-type galaxies in the local Universe is responsible for absorbing approximately one third of the energy emitted by stars. It is often assumed that dust heating is mainly attributable to the absorption of ultraviolet and optical p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2127::f115d9e910065b5e093cb173ebb8996a
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3068729
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3068729
The star formation rate and the mass of interstellar medium (ISM) have a high predictive power for the future evolution of a galaxy. Nevertheless, deriving such properties is not straightforward. Dust emission, an important diagnostic of star formati
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2127::c16ce96be5f87e8a3585b26ef5d964fd
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3068715
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3068715
We compare the spectral energy distributions (SEDs) and inferred physical properties for simulated and observed galaxies at low redshift. We exploit UV-submillimetre mock fluxes of ∼7000 z = 0 galaxies from the EAGLE suite of cosmological simulatio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2127::4faab43d6a4a644c8e2795cc7dae06fd
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3068808
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3068808
Context. Dust plays an important role in shaping a galaxy's spectral energy distribution (SED). It absorbs ultraviolet (UV) to near-infrared radiation and re-emits this energy in the far-infrared (FIR). The FIR is essential to understand dust in gala
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2127::e9a5b008d18da3d39f3c29a8e3d4a92c
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3068782
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3068782
Autor:
S. Bordon, A. Bajat, B. Houret, O. Godet, V. Waegebaert, S. Delaigue, C. Amoros, S. Maestre, W. Marty, P. Mandrou, R. Pons, D. Rambaud, Jean-Luc Atteia, K. Lacombe, P. Ramon, M. Galliano
Publikováno v:
Experimental Astronomy. 46:337-356
French (CNES) and Chinese (CNSA) space agencies collaborate to build the SVOM (Space-based multi-band Variable Object Monitor) mission due to be launched in 2021 to study gamma-ray bursts and high-energy transients. The SVOM prime instrument, ECLAIRs
Aims. We compare the far-infrared to sub-millimetre dust emission properties measured in high Galactic latitude cirrus with those determined in a sample of 204 late-type DustPedia galaxies. The aim is to verify if it is appropriate to use Milky Way d
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2127::2e62e262899963167efc661f54363782
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3068871
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3068871