1
“...After almost 60 years since the discovery of the first pulsar, the physics of Neutron Stars (NSs...”
The masses of Neutron Stars
Tese
3
4
Assuntos:
“...Be stars...”
BeAtlas: A grid of synthetic spectra for Be stars - Bayesian inference of the physical properties of B and Be Stars
Tese
5
“...About 10% of the known massive stars have a magnetic field of relevant strength. Combined with the...”
Magnetospheres around High Mass Stars revealed by Polarimetry
Dissertação
8
“...White dwarf stars are the most common final stage of stellar evolution, corresponding to 99% of all...”
Asteroseismology of pulsating low-mass white dwarf stars
Tese
9
Assuntos:
“...Ultracompact stars...”
On the possibility of ultracompact stars in semiclassical gravity
Tese
10
11
“... 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
12
Assuntos:
“...neutron stars...”
Population study of radio-quiet and thermally emitting isolated neutron stars
Tese
13
“...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
14
Assuntos:
“...Stellar populations; Stellar spectra; Stellar atmosphere; Subdwarf stars...”
Hot Subdwarf stars in the integrated light of old stellar populations
Tese
15
Assuntos:
“...Neutron stars...”
General Relativisti Study of the Stru ture of Highly Magnetized Neutron Stars
Tese