Evidence for the Accretion of Gas in Star-forming Galaxies: High N/O Abundances in Regions of Anomalously Low Metallicity

Yuanze Luo, Timothy Heckman, Hsiang Chih Hwang, Kate Rowlands, Laura Sánchez-Menguiano, Rogério Riffel, Dmitry Bizyaev, Brett H. Andrews, José G. Fernández-Trincado, Niv Drory, Jorge Sánchez Almeida, Roberto Maiolino, Richard R. Lane, MARIA DEL CARMEN ARGUDO FERNANDEZ

Resultado de la investigación: Contribución a una revistaArtículorevisión exhaustiva

5 Citas (Scopus)

Resumen

While all models for the evolution of galaxies require the accretion of gas to sustain their growth via on-going star formation, it has proven difficult to directly detect this inflowing material. In this paper we use data of nearby star-forming galaxies in the SDSS IV Mapping Nearby Galaxies at Apache Point Observatory survey to search for evidence of accretion imprinted in the chemical composition of the interstellar medium. We measure both the O/H and N/O abundance ratios in regions previously identified as having anomalously low values of O/H. We show that the unusual locations of these regions in the N/O versus O/H plane indicate that they have been created through the mixing of disk gas having higher metallicity with accreted gas having lower metallicity. Taken together with previous analysis on these anomalously low-metallicity regions, these results imply that accretion of metal-poor gas can probably sustain star formation in present-day late-type galaxies.

Idioma originalInglés
Número de artículo183
PublicaciónAstrophysical Journal
Volumen908
N.º2
DOI
EstadoPublicada - 20 feb. 2021
Publicado de forma externa

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