The H α star formation main sequence in cluster and field galaxies at z ∼1.6

Vista sencilla de ítem
dc.contributor.authorNantais J.
dc.contributor.authorWilson G.
dc.contributor.authorMuzzin A.
dc.contributor.authorOld L.J.
dc.contributor.authorDemarco R.
dc.contributor.authorCerulo P.
dc.contributor.authorBalogh M.
dc.contributor.authorRudnick G.
dc.contributor.authorChan J.
dc.contributor.authorCooper M.C.
dc.contributor.authorForrest B.
dc.contributor.authorHayden B.
dc.contributor.authorLidman C.
dc.contributor.authorNoble A.
dc.contributor.authorPerlmutter S.
dc.contributor.authorRhea C.
dc.contributor.authorSurace J.
dc.contributor.authorVan Der Burg R.
dc.contributor.authorVan Kampen E.
dc.date.accessioned2021-08-26T19:45:37Z
dc.date.available2021-08-26T19:45:37Z
dc.date.issued2020-12
dc.descriptionIndexación Scopuses
dc.description.abstractWe calculate H α-based star formation rates and determine the star formation rate-stellar mass relation for members of three Spitzer Adaptation of the Red-Sequence Cluster Survey (SpARCS) clusters at z ∼1.6 and serendipitously identified field galaxies at similar redshifts to the clusters. We find similar star formation rates in cluster and field galaxies throughout our range of stellar masses. The results are comparable to those seen in other clusters at similar redshifts, and consistent with our previous photometric evidence for little quenching activity in clusters. One possible explanation for our results is that galaxies in our z ∼1.6 clusters have been accreted too recently to show signs of environmental quenching. It is also possible that the clusters are not yet dynamically mature enough to produce important environmental quenching effects shown to be important at low redshift, such as ram-pressure stripping or harassment. © 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society.es
dc.description.urihttps://academic-oup-com.recursosbiblioteca.unab.cl/mnras/article/499/3/3061/5913329
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, Volume 499, Issue 3, Pages 3061 - 30701 December 2020es
dc.identifier.doi10.1093/mnras/staa2872
dc.identifier.issn00358711
dc.identifier.urihttp://repositorio.unab.cl/xmlui/handle/ria/20002
dc.language.isoenes
dc.publisherOxford University Presses
dc.subjectStar Formationes
dc.subjectGalaxieses
dc.subjectGalactic Evolutiones
dc.titleThe H α star formation main sequence in cluster and field galaxies at z ∼1.6es
dc.typeArtículoes
Archivos
Bloque original
Mostrando 1 - 1 de 1
Miniatura
Nombre:
Nantais_J_The_H_α_star_2020.pdf
Tamaño:
798.35 KB
Formato:
Adobe Portable Document Format
Descripción:
TEXTO COMPLETO EN INGLÉS
Descargar
Bloque de licencias
Mostrando 1 - 1 de 1
No hay miniatura disponible
Nombre:
license.txt
Tamaño:
1.71 KB
Formato:
Item-specific license agreed upon to submission
Descripción:
Descargar
Colecciones
FCE - Artículos de Revista