The paschen discontinuity in B stars

Measurements of the Paschen discontinuity in stars withT eff ≥104K leads to the conclusion that the D P/DB ratio increases with temperature faster than expected. The increase of D P/DB with (logg)−1 is also steep.

Guardado en:
Detalles Bibliográficos
Autor principal: Ringuelet, Adela Emilia
Formato: Articulo
Lenguaje:Inglés
Publicado: 1969
Materias:
Astronomía
Ciencias Astronómicas
Paschen discontinuity
Balmer discontinuity
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/131085
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata
id I19-R120-10915-131085
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Astronomía
Ciencias Astronómicas
Paschen discontinuity
Balmer discontinuity
spellingShingle Astronomía
Ciencias Astronómicas
Paschen discontinuity
Balmer discontinuity
Ringuelet, Adela Emilia
The paschen discontinuity in B stars
topic_facet Astronomía
Ciencias Astronómicas
Paschen discontinuity
Balmer discontinuity
description Measurements of the Paschen discontinuity in stars withT eff ≥104K leads to the conclusion that the D P/DB ratio increases with temperature faster than expected. The increase of D P/DB with (logg)−1 is also steep.
format Articulo
Articulo
author Ringuelet, Adela Emilia
author_facet Ringuelet, Adela Emilia
author_sort Ringuelet, Adela Emilia
title The paschen discontinuity in B stars
title_short The paschen discontinuity in B stars
title_full The paschen discontinuity in B stars
title_fullStr The paschen discontinuity in B stars
title_full_unstemmed The paschen discontinuity in B stars
title_sort paschen discontinuity in b stars
publishDate 1969
url http://sedici.unlp.edu.ar/handle/10915/131085
work_keys_str_mv AT ringueletadelaemilia thepaschendiscontinuityinbstars
AT ringueletadelaemilia paschendiscontinuityinbstars
bdutipo_str Repositorios
_version_ 1764820453269962753

Ejemplares similares