Results 71 to 80 of about 86,432 (192)

Conceitos de Astronomia: Análise a partir de textos escritos pelos alunos

open access: yesRevista de Ensino de Ciências e Matemática, 2020
Esta pesquisa foi realizada com alunos da primeira série do Ensino Médio de uma escola pública do Estado de São Paulo, em aulas de Física. Esses alunos participaram de uma atividade em que deveriam elaborar, em grupo, a escrita de uma história relativa ...
Idmaura Calderaro Martins Galvão   +1 more
doaj   +1 more source

Low‐Energy Atomic Scattering: S‐Wave Relation Between the Interaction Potential and the Phase Shift

open access: yesAnnalen der Physik, Volume 537, Issue 11, November 2025.
The validity of the on‐shell approximation for s‐wave scattering is examined across one, two, and three dimensions using exactly solvable model interaction potentials. By comparing exact and approximate s‐wave components of the interaction potential, the analysis reveals that the approximation improves with increasing momentum and decreasing ...
Francesco Lorenzi, Luca Salasnich
wiley   +1 more source

Xarxes internacionals d'art, ciència i tecnologia

open access: yesArtnodes, 2007
Durant aquesta conversa, Roger Malina reflexiona sobre la relació entre art, ciència i tecnologia, considerant-les no com a disciplines independents sinó connectades i que comparteixen els mateixos mitjans.
Roger Malina
doaj   +1 more source

JWST Imaging of the Closest Globular Clusters—VI. The Lowest‐Mass Objects in M 4 and the Galactic Bulge

open access: yesAstronomische Nachrichten, Volume 346, Issue 9, November 2025.
ABSTRACT We present James Webb Space Telescope observations of M 4—the closest globular cluster—that probe the lower Main Sequence down to the hydrogen‐burning limit. The unveiled stellar sequence reaches much fainter luminosities than previously possible, revealing a few extremely red objects that are consistent with brown dwarfs as cool as Teff∼1000K$
L. R. Bedin   +10 more
wiley   +1 more source

Simultaneous multi-wavelength observations of microquasars (the MINE collaboration)

open access: yes, 2003
We present the international collaboration MINE (Multi-lambda INTEGRAL NEtwork) aimed at conducting multi-wavelength observations of microquasars simultaneously with the INTEGRAL satellite.
Brown, I.   +11 more
core  

The Araucaria Project. First Cepheid Distance to the Sculptor Group Galaxy NGC 7793 from Variables discovered in a Wide-Field Imaging Survey

open access: yes, 2010
We have detected, for the first time, Cepheid variables in the Sculptor Group spiral galaxy NGC 7793. From wide-field images obtained in the optical V and I bands on 56 nights in 2003-2005, we have discovered 17 long-period (24-62 days) Cepheids whose ...
Alejandro Garcia-Varela   +41 more
core   +1 more source

Życie i działalność naukowa Tadeusza Banachiewicza

open access: yesStudia Historiae Scientiarum, 2016
Niniejszy artykuł jest syntetyczną biografią Tadeusza Banachiewicza (1882–1954), uwzględniającą jego najważniejsze wyniki naukowe.
Renata Bujakiewicz-Korońska   +1 more
doaj   +1 more source

Detailed atmospheric abundance analysis of the optical counterpart of the IR source IRAS 16559-2957 [PDF]

open access: yes, 2013
We have undertaken a detailed abundance analysis of the optical counterpart of the IR source IRAS16559-2957 with the aim of confirming its possible post-AGB nature.
Ferro, A. Arellano, Molina, R. E.
core  

ALGUMAS TENDÊNCIAS DAS PUBLICAÇÕES RELACIONADAS À ASTRONOMIA EM PERIÓDICOS BRASILEIROS DE ENSINO DE FÍSICA NAS ÚLTIMAS DÉCADAS

open access: yesEnsaio Pesquisa em Educação em Ciências, 2010
Apresentamos neste artigo uma análise sobre as publicações relacionadas à Astronomia nas últimas décadas, presentes em dois periódicos de ensino de Física no país: o Caderno Brasileiro de Ensino de Física e a Revista Brasileira de Ensino de Física. Pelos
Gustavo Iachel, Roberto Nardi
doaj  

3D numerical model of the Omega Nebula (M17): simulated thermal X-ray emission

open access: yes, 2009
We present 3D hydrodynamical simulations of the superbubble M17, also known as the Omega nebula, carried out with the adaptive grid code yguazu'-a, which includes radiative cooling. The superbubble is modelled considering the winds of 11 individual stars
A. Esquivel   +44 more
core   +1 more source

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