Influence of mid-infrared Galactic bubble on surroundings: A case study on IRAS 16489-4431

Fuente: arXiv
Guardado en:
Detalles Bibliográficos
Autores principales: Hoque, Ariful, Baug, Tapas, Dewangan, Lokesh, Wang, Ke, Liu, Tie, Mondal, Soumen
Formato: Preprint
Publicado: 2024
Materias:
Acceso en línea:
Etiquetas: Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
_version_ 1866929362046025728
author Hoque, Ariful
Baug, Tapas
Dewangan, Lokesh
Wang, Ke
Liu, Tie
Mondal, Soumen
author_facet Hoque, Ariful
Baug, Tapas
Dewangan, Lokesh
Wang, Ke
Liu, Tie
Mondal, Soumen
contents We studied the influence of a massive star on a mid-infrared bubble and its surrounding gas in the IRAS\,16489-4431 star-forming region using multi-wavelength data. The {\it Spitzer} mid-infrared band images revealed the shocked nature of the bubble. Analyses showed that the bubble is developed by a massive star owing to its strong radiation pressure. Evidence of collected material along the edge of the bubble was noted by the cold gas tracer line observed using Atacama Millimeter/submillimeter Array (ALMA). The presence of dense dust cores with bi-polar outflows and young stellar objects toward the collected material is suggestive of active star formation possibly influenced by the expansion of the radiation driven bubble.
format Preprint
id arxiv_https___arxiv_org_abs_2405_17993
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Influence of mid-infrared Galactic bubble on surroundings: A case study on IRAS 16489-4431
Hoque, Ariful
Baug, Tapas
Dewangan, Lokesh
Wang, Ke
Liu, Tie
Mondal, Soumen
Astrophysics of Galaxies
We studied the influence of a massive star on a mid-infrared bubble and its surrounding gas in the IRAS\,16489-4431 star-forming region using multi-wavelength data. The {\it Spitzer} mid-infrared band images revealed the shocked nature of the bubble. Analyses showed that the bubble is developed by a massive star owing to its strong radiation pressure. Evidence of collected material along the edge of the bubble was noted by the cold gas tracer line observed using Atacama Millimeter/submillimeter Array (ALMA). The presence of dense dust cores with bi-polar outflows and young stellar objects toward the collected material is suggestive of active star formation possibly influenced by the expansion of the radiation driven bubble.
title Influence of mid-infrared Galactic bubble on surroundings: A case study on IRAS 16489-4431
topic Astrophysics of Galaxies
url https://arxiv.org/abs/2405.17993