Results 41 to 50 of about 136,231 (311)
The reclassification of NSV 1586 from a suspected Cepheid star to a UG class system [PDF]
On 2018 August 9, a contribution to the VSNET mailing list suggested that due to certain photometric attributes, NSV 1586 could possibly belong to the Dwarf Nova (DN) class.
Galdies, Charles +3 more
core
This is the triennial report of IAU Commission 27, mostly presenting a review of recent advances in the field.
Handler, G. +12 more
+5 more sources
ABSTRACT Immune effector cell‐associated hemophagocytic lymphohistiocytosis‐like syndrome (IEC‐HS) is a life‐threatening hyperinflammatory toxicity distinct from cytokine release syndrome (CRS) and neurotoxicity following chimeric antigen receptor T‐cell (CAR‐T) therapy. In a single‐institution retrospective cohort of pediatric and young adult patients
Thomas J. Galletta +6 more
wiley +1 more source
Discovery of the most compact 3+1-type quadruple star system TIC 120362137
Hierarchical multiple stellar systems with short outer periods comprise an important subgroup of multiple star systems. In this paper we present the discovery and spectro-photodynamical analysis of the most compact known 3+1 quadruple stellar system, TIC
Tamás Borkovits +20 more
doaj +1 more source
The Role of Hematopoietic Cell Transplantation in Ataxia‐Telangiectasia
ABSTRACT Background Ataxia‐telangiectasia (A‐T) is a DNA repair disorder characterized by neurodegeneration, immunodeficiency, and cancer predisposition. Hematopoietic cell transplantation (HCT) is an established therapy in related disorders such as Fanconi anemia (FA) and Nijmegen breakage syndrome (NBS), but its role in A‐T is unclear.
Laila Alkhouli +3 more
wiley +1 more source
Synergies between exoplanet surveys and variable star research
With the discovery of the first transiting extrasolar planetary system back in 1999, a great number of projects started to hunt for other similar systems. Because the incidence rate of such systems was unknown and the length of the shallow transit events
Kovacs Geza
doaj +1 more source
A new red variable star in the globular cluster M4
G302 = L3107 is a red star located at the lowest end of the red giant branch of the globular cluster M4. According to its location on the GM diagram, G302 may be a cluster member.
Sheng, CJ, Lin, Q, Zhang, CS, Yao, BA
core +1 more source
Sparse Identification of Variable Star Dynamics
Variable stars play a crucial role as standard candles and provide valuable insights into stellar physics. They can be modeled either through fully fledged hydrodynamical simulations or analytically as systems of coupled differential equations describing
Mario Pasquato +8 more
core +1 more source
Variable stars of short period.
Reprinted from the Proceedings of the American academy of arts and sciences, vol. XVI. ; Mode of access: Internet.
openaire +2 more sources

