Results 141 to 150 of about 3,849,349 (342)
Fundamental Parameters for Central Stars of 103 Infrared Bow Shock Nebulae
Stellar bow shock nebulae are arcuate shock fronts formed by the interaction of radiation-driven stellar winds and the relative motion of the ambient interstellar material.
Nikhil Patten +18 more
doaj +1 more source
Oxygen and helium abundances in Galactic H II regions -- II. Abundance gradients [PDF]
L. Deharveng +3 more
openalex +1 more source
H II regions in peculiar galaxies
A survey of 32 galaxies, either classified as peculiar or having peculiar distributions of H ii regions, is presented in order to ascertain the range of the peculiarities and the degree to which they are similar. Ten different types are recognized, several of which are interrelated.
openaire +1 more source
Adaptaquin selectively kills glioma stem cells while sparing differentiated brain cells. Transcriptomic and proteomic analyses show Adaptaquin disrupts iron and cholesterol homeostasis, with iron chelation amplifying cytotoxicity via cholesterol depletion, mitochondrial dysfunction, and elevated reactive oxygen species.
Adrien M. Vaquié +16 more
wiley +1 more source
The MDW Hα Sky Survey: Data Release 1
The Mittelman–di Cicco–Walker (MDW) H α Sky Survey is an autonomously operated all-sky narrowband (3 nm) H α imaging survey. The survey was founded by amateur astronomers, and the northern sky (decl.
Noor Aftab +8 more
doaj +1 more source
The dust properties of bubble H II regions as seen byHerschel [PDF]
L. D. Anderson +12 more
openalex +1 more source
Theoretical models for H II regions. II - The extragalactic H II region abundance sequence
M. A. Dopita, I. N. Evans
openaire +1 more source
This study integrates transcriptomic profiling of matched tumor and healthy tissues from 32 colorectal cancer patients with functional validation in patient‐derived organoids, revealing dysregulated metabolic programs driven by overexpressed xCT (SLC7A11) and SLC3A2, identifying an oncogenic cystine/glutamate transporter signature linked to ...
Marco Strecker +16 more
wiley +1 more source
The carbon-to-oxygen (C/O) abundance ratio is a valuable tracer of star formation history, as C and O enrichment occurs on different timescales. However, measurements based on ultraviolet (UV) collisionally excited lines and those based on optical ...
Paige M. Kelly +7 more
doaj +1 more source
Massive Star Formation in Luminous Infrared Galaxies: Giant H [CSC]ii[/CSC] Regions and Their Relation to Super–Star Clusters [PDF]
A. Alonso‐Herrero +3 more
openalex +1 more source

