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Autores principales: Chung, Jiwon, Lee, Joon Hyeop, Jeong, Hyunjin
Formato: Preprint
Publicado: 2024
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Acceso en línea:https://arxiv.org/abs/2406.07783
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author Chung, Jiwon
Lee, Joon Hyeop
Jeong, Hyunjin
author_facet Chung, Jiwon
Lee, Joon Hyeop
Jeong, Hyunjin
contents We present novel insights into the interplay between tidal forces and star formation in interacting galaxies before their first pericentre passage. We investigate seven close pair galaxies devoid of visible tidal disturbances, such as tails, bridges, and shells. Using integral field spectroscopy (IFS) data of extended Calar Alto Legacy Integral Field Area (eCALIFA), we unveil a previously unreported phenomenon: H alhpa emission, a proxy for recent star formation, exhibits a significant enhancement in regions facing the companion galaxy, reaching up to 1.9 times higher flux compared to opposite directions. Notably, fainter companions within pairs display a more pronounced one-sided H alpha excess, exceeding the typical range observed in isolated galaxies with 2 sigma confidence level. Furthermore, the observed H alpha excess in fainter companion galaxies exhibits a heightened prominence at the outer galactic regions. These findings suggest that tidal forces generated before the first pericentre passage exert a stronger influence on fainter galaxies due to their shallower potential wells by their brighter companions. This unveils a more intricate interplay between gravitational interactions and star formation history within interacting galaxies than previously understood, highlighting the need further to explore the early stages of interaction in galaxy evolution.
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spellingShingle One-sided H alpha Excess before the First Pericentre Passage in Galaxy Pairs
Chung, Jiwon
Lee, Joon Hyeop
Jeong, Hyunjin
Astrophysics of Galaxies
We present novel insights into the interplay between tidal forces and star formation in interacting galaxies before their first pericentre passage. We investigate seven close pair galaxies devoid of visible tidal disturbances, such as tails, bridges, and shells. Using integral field spectroscopy (IFS) data of extended Calar Alto Legacy Integral Field Area (eCALIFA), we unveil a previously unreported phenomenon: H alhpa emission, a proxy for recent star formation, exhibits a significant enhancement in regions facing the companion galaxy, reaching up to 1.9 times higher flux compared to opposite directions. Notably, fainter companions within pairs display a more pronounced one-sided H alpha excess, exceeding the typical range observed in isolated galaxies with 2 sigma confidence level. Furthermore, the observed H alpha excess in fainter companion galaxies exhibits a heightened prominence at the outer galactic regions. These findings suggest that tidal forces generated before the first pericentre passage exert a stronger influence on fainter galaxies due to their shallower potential wells by their brighter companions. This unveils a more intricate interplay between gravitational interactions and star formation history within interacting galaxies than previously understood, highlighting the need further to explore the early stages of interaction in galaxy evolution.
title One-sided H alpha Excess before the First Pericentre Passage in Galaxy Pairs
topic Astrophysics of Galaxies
url https://arxiv.org/abs/2406.07783