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stars and » status and (Expandir a busca), states and (Expandir a busca), starch and (Expandir a busca)
1
“... prediction for the final stage of rotational evolution is synchronism for the case of circular orbits and...”
Equilibrium Tides on Planets and Stars
Tese
2
Assuntos:
“...Be stars...”
BeAtlas: A grid of synthetic spectra for Be stars - Bayesian inference of the physical properties of B and Be Stars
Tese
3
“... for 11 elements, taking into account the evolution of Population III and II stars and the transition between...”
The role of population II and III stars in the cosmic chemical evolution
Dissertação
4
Assuntos:
“...neutron stars...”
Population study of radio-quiet and thermally emitting isolated neutron stars
Tese
5
“...Even after 80 years of intense research, the composition of neutron stars remains unknown, since...”
Different approaches to the Composition of Neutron Stars and their Environment
Tese
6
7
“... dwarfs, exploring the evolution of hydrogen-rich and hydrogen-deficient white dwarfs stars with masses...”
Evolutionary sequences for H and He atmosphere massive white dwarf stars
Dissertação
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10
“...After almost 60 years since the discovery of the first pulsar, the physics of Neutron Stars (NSs...”
The masses of Neutron Stars
Tese
11
12
Assuntos:
“...Binary stars...”
The rotational evolution of Sun-like stars and the influence of low-mass binary companions
Dissertação
13
Assuntos:
“...Stars: kinematics and dynamics...”
Formation and evolution of globular clusters in the Galaxy and Magellanic Clouds
Tese
14
Assuntos:
“...Stars: Abundances...”
Differential abundances in metal-poor stars: impact in the study of the Galaxy, stellar evolution and Big Bang nucleosynthesis
Tese
15
“... of 18 stars were carried out int the V and R filters. We improved the fitting method of the D+D model...”
Magnetospheres around High Mass Stars revealed by Polarimetry
Dissertação
16
“... pulsating low-mass white dwarf stars have stellar masses between 0.30 M⊙ and 0.45 M⊙ and show photometric...”
Asteroseismology of pulsating low-mass white dwarf stars
Tese
18
19
Assuntos:
“...Ultracompact stars...”
On the possibility of ultracompact stars in semiclassical gravity
Tese
20
Assuntos:
“...Be stars...”
Searching for Be stars using multi-band photometry: Case study of NGC330 using SOAR and S-PLUS data
Dissertação