Ongoing studies of different groups of stars result in improving our knowledge of their fundamental parameters and evolutionary status. Also, they result in finding new phases of stellar evolution, which require theoretical explanation. At the same time,
Miroshnichenko Anatoly S. +9 more
doaj +1 more source
Newly discovered Wolf-Rayet and weak emission-line central stars of planetary nebulae [PDF]
We present the spectra of 32 previously unpublished confirmed and candidate Wolf-Rayet ([WR]) and weak emission-line (WELS) central stars of planetary nebulae (CSPNe).
Miszalski, B +7 more
core +1 more source
Predictive Ability of Plasma p‐tau217 for β‐Amyloid Status: A Prospective Multicenter Study
ABSTRACT Objective Plasma tau phosphorylated at threonine 217 (p‐tau217) measured with fully automated platforms has shown high accuracy for Alzheimer's disease (AD) diagnosis, but real‐world multicenter data remain limited. We aimed to validate the diagnostic performance of p‐tau217 for identifying AD pathology in a real‐world multicenter cohort ...
Miquel Massons +33 more
wiley +1 more source
Models of circumstellar molecular radio line emission: Mass loss rates for a sample of bright carbon stars [PDF]
F. L. Schoeier, H. Olofsson
openalex +1 more source
Predicting the observability of population III stars with ELT-HARMONI via the helium 1640 Å emission line [PDF]
Kearn Grisdale +7 more
openalex +1 more source
Thin accretion discs around neutron and quark stars [PDF]
The possibility of observationally discriminating between various types of neutron stars, described by different equations of state of the nuclear matter, as well as differentiating neutron stars from other types of exotic objects, for example, quark ...
Harko, T +5 more
core +1 more source
Persistent Bilateral [18F]THK5351 and Migrating Unilateral [18F]FDG Uptake in Anti‐LGI1 Encephalitis
ABSTRACT Anti–leucine‐rich glioma‐inactivated 1 encephalitis (LGI1‐E) can cause persistent cognitive deficits, but the mechanisms remain unclear. A 40‐year‐old woman with LGI1‐E presented with subacute cognitive deficits and showed mild left medial temporal lobe (MTL) swelling and fluid‐attenuated inversion recovery (FLAIR) hyperintensity on initial ...
Yusuke Akitomi +8 more
wiley +1 more source
ExoplaNeT accRetion mOnitoring sPectroscopic surveY (ENTROPY)
Context. Observations of helium emission lines from classical T Tauri stars at high resolution (Rλ > 10 000) offer great potential, showing distinct profile characteristics that help probe regions within the accretion geometry untapped by hydrogen lines.
Viswanath Gayathri +10 more
doaj +1 more source
Weak emission line central stars of planetary nebulae
To understand the evolution and morphology of planetary nebulae, a detailed knowledge of their central stars is required. Central stars that exhibit emission lines in their spectra, indicating stellar mass-loss allow to study the evolution of planetary ...
Peña, Miriam +5 more
core
Properties of Regions Forming the FeII Emission Lines in Be Stars
We study FeII and Balmer hydrogen emission lines observed simultaneously of 18 southern Be stars. We use the self-absorption-curve method (SAC) to determine the optical depth regime of FeII emission lines and to derive first insights on the physical properties of their forming regions.
Arias, Maria Laura +3 more
openaire +3 more sources

