S-type star - significado y definición. Qué es S-type star
Diclib.com
Diccionario ChatGPT
Ingrese una palabra o frase en cualquier idioma 👆
Idioma:

Traducción y análisis de palabras por inteligencia artificial ChatGPT

En esta página puede obtener un análisis detallado de una palabra o frase, producido utilizando la mejor tecnología de inteligencia artificial hasta la fecha:

  • cómo se usa la palabra
  • frecuencia de uso
  • se utiliza con más frecuencia en el habla oral o escrita
  • opciones de traducción
  • ejemplos de uso (varias frases con traducción)
  • etimología

Qué (quién) es S-type star - definición


S-type star         
  • TP-AGB]] to become an S star and then a [[carbon star]]<ref name=weiss/>
  • PIONIER]] on the VLT
COOL GIANT WITH APPROXIMATELY EQUAL QUANTITIES OF CARBON AND OXYGEN IN ITS ATMOSPHERE
Extrinsic S-type star; Intrinsic S star; Extrinsic S star; MS star (spectral type)
An S-type star (or just S star) is a cool giant with approximately equal quantities of carbon and oxygen in its atmosphere. The class was originally defined in 1922 by Paul Merrill for stars with unusual absorption lines and molecular bands now known to be due to s-process elements.
O-type star         
  • CNO cycle that powers massive O-type stars.
  • The O-type star in Cepheus B, HD 217086, illuminates the molecular cloud with ultraviolet radiation, driving it back while compressing it, triggering the formation of new stars.
  • The [[Trifid Nebula]] (M20) is sculpted and lit by the luminous O7.5III star visible at its centre in this infrared image.
  • The central star of NGC 6826 is a low-mass O6 star.
  • Alnitak is a triple star system with an O9.7 supergiant and an O9 giant as well as a B0 giant. These stars illuminate the nearby [[Flame Nebula]].
  • Structure of low-mass, intermediate-mass, and high-mass stars. M indicates [[solar mass]]es.
  • Evolutionary tracks on the HR diagram. The 15{{Solar mass}} and 60{{Solar mass}} tracks are typical of massive O-type stars.
  • sdO-type star cross-section showing inert core and helium shell burning
  • The brightest star in the [[Trapezium cluster]] is O7V star θ1 Orionis C. The other three are B0.5 and B1 main-sequence stars.
STELLAR CLASSIFICATION
O star; Type-O star; O-type Stars; O-type stars
An O-type star is a hot, blue-white star of spectral type O in the Yerkes classification system employed by astronomers. They have temperatures in excess of 30,000 kelvin (K).
Carbon star         
  • Echelle spectra]] of the carbon star [[UU Aurigae]]
  • LMC]] carbon stars with a given near-infrared luminosity. The median value is marked in red. Adapted from Ripoche ''et al.'' (2020)<ref name="RipocheMNRAS495"/>
STAR WHOSE ATMOSPHERE CONTAINS MORE CARBON THAN OXYGEN
Carbon Star; Type-C stars; Carbon stars; N star; H star; Hd star; Carbon Stars; C star; Oxygen star; C-type star; Carbon giant; Type-R star
A carbon star (C-type star) is typically an asymptotic giant branch star, a luminous red giant, whose atmosphere contains more carbon than oxygen. The two elements combine in the upper layers of the star, forming carbon monoxide, which consumes most of the oxygen in the atmosphere, leaving carbon atoms free to form other carbon compounds, giving the star a "sooty" atmosphere and a strikingly ruby red appearance.