Initial-Final Mass Relationship for Stars of Different Metallicities
Following Paczy\'{n}ski & Zi\'{o}lkowski (1968) and Han et al. (1994), we assume that the envelope of an asymptotic giant branch (AGB) or a first giant branch (FGB) star is lost when the binding energy of the envelope is equal to zero ($\Delta W=0$) and ...
Alcock +109 more
core +1 more source
Discovery of photospheric argon in very hot central stars of planetary nebulae and white dwarfs [PDF]
We report the first discovery of argon in hot evolved stars and white dwarfs. We have identified the ArVII 1063.55A line in some of the hottest known (Teff=95000-110000 K) central stars of planetary nebulae and (pre-) white dwarfs of various spectral ...
Barstow +30 more
core +2 more sources
Searching for Ultra-light Dark Matter in Spatial Correlations of White Dwarf Structure
If dark matter is ultra-light and has certain Standard Model interactions, it can change the mass–radius relation of white dwarf (WD) stars. The coherence length of ultra-light dark matter (ULDM) imparts spatial correlations in deviations from the ...
Nicole R. Crumpler +3 more
doaj +1 more source
Um antropófago em Hollywood: Oswald espectador de Valentino
Retomando um caso emblemático das referências, pouco exploradas, do modernismo brasileiro a Hollywood, o de Oswald de Andrade ao ator Rudolph Valentino (um dos primeiros super-stars), pretende-se analisar como a temática da reprodução das imagens pelo ...
Alexandre André Nodari
doaj +1 more source
ABSTRACT Purpose Although not always achieved, complete chemotherapy‐induced nausea and vomiting (CINV) control is the conventional goal of CINV prophylaxis. In this two‐center, mixed‐methods study, we sought to understand the preferences of adolescent patients and family caregivers for CINV control endpoints.
Haley Newman +8 more
wiley +1 more source
A Highly Magnetic Ultramassive White Dwarf with a 23 minute Rotation Period
We present a physical characterization of Tsinghua University-Ma Huateng Telescope for Survey (TMTS) J00063798+3104160 (J0006), a rapidly rotating, ultramassive white dwarf (WD) identified in high-cadence light curves from the TMTS.
Jincheng Guo +19 more
doaj +1 more source
A star is dead: Kim Novak, Vertigo e a autocrítica do star system hollywoodiano
O artigo analisa Vertigo (1958), de Alfred Hitchcock, do ponto de vista do star system hollywoodiano e das relações de força que produtores e diretores estabelecem com as estrelas da indústria cinematográfica.
Luiz Carlos Oliveira Jr.
doaj +1 more source
The Gemini Planet Imager Exoplanet Survey: Giant Planet and Brown Dwarf Demographics From 10-100 AU
We present a statistical analysis of the first 300 stars observed by the Gemini Planet Imager Exoplanet Survey (GPIES). This subsample includes six detected planets and three brown dwarfs; from these detections and our contrast curves we infer the ...
Ammons, S. Mark +65 more
core +3 more sources
Photometric and Spectroscopic Analysis of Cool White Dwarfs with Trigonometric Parallax Measurements [PDF]
A photometric and spectroscopic analysis of 152 cool white dwarf stars is presented. The discovery of 7 new DA white dwarfs, 2 new DQ white dwarfs, 1 new magnetic white dwarf, and 3 weak magnetic white dwarf candidates, is reported, as well as 19 known ...
Borysow A. +9 more
core +2 more sources
Intravitreal GD2‐Specific Chimeric Antigen Receptor T‐Cell Therapy for Refractory Retinoblastoma
ABSTRACT Effective treatments for advanced, treatment‐resistant retinoblastoma (RB) remain limited. GD2‐specific chimeric antigen receptor (CAR) T cells show potent antitumor activity with minimal toxicity but have not previously been evaluated in RB.
Subongkoch Subhadhirasakul +13 more
wiley +1 more source

