Stellar tidal streams around nearby spiral galaxies with deep imaging from amateur telescopes

Fuente: arXiv
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Auteurs principaux: Martinez-Delgado, David, Stein, Michael, Sakowska, Joanna D., Weigelt, M. Maurice, Roman, Javier, Donatiello, Giuseppe, Roca-Fabrega, Santi, Schirmer, Mischa, Grebel, Eva K., Saifollahi, Teymoor, Kanipe, Jeff, Gomez-Flechoso, M. Angeles, Akhlaghi, Mohammad, Javanmardi, Behnam, Wu, Gang, Eskandarlou, Sepideh, Bomans, Dominik J., Henkel, Cristian, Block, Adam, Hanson, Mark, Schedler, Johannes, Teuwen, Karel, GaBany, R. Jay, Perez, Alvaro Ibañez, Crawford, Ken, Promper, Wolfgang, Jimenez, Manuel, Farras-Aloy, Silvia, Miro-Carretero, Juan
Format: Preprint
Publié: 2025
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author Martinez-Delgado, David
Stein, Michael
Sakowska, Joanna D.
Weigelt, M. Maurice
Roman, Javier
Donatiello, Giuseppe
Roca-Fabrega, Santi
Schirmer, Mischa
Grebel, Eva K.
Saifollahi, Teymoor
Kanipe, Jeff
Gomez-Flechoso, M. Angeles
Akhlaghi, Mohammad
Javanmardi, Behnam
Wu, Gang
Eskandarlou, Sepideh
Bomans, Dominik J.
Henkel, Cristian
Block, Adam
Hanson, Mark
Schedler, Johannes
Teuwen, Karel
GaBany, R. Jay
Perez, Alvaro Ibañez
Crawford, Ken
Promper, Wolfgang
Jimenez, Manuel
Farras-Aloy, Silvia
Miro-Carretero, Juan
author_facet Martinez-Delgado, David
Stein, Michael
Sakowska, Joanna D.
Weigelt, M. Maurice
Roman, Javier
Donatiello, Giuseppe
Roca-Fabrega, Santi
Schirmer, Mischa
Grebel, Eva K.
Saifollahi, Teymoor
Kanipe, Jeff
Gomez-Flechoso, M. Angeles
Akhlaghi, Mohammad
Javanmardi, Behnam
Wu, Gang
Eskandarlou, Sepideh
Bomans, Dominik J.
Henkel, Cristian
Block, Adam
Hanson, Mark
Schedler, Johannes
Teuwen, Karel
GaBany, R. Jay
Perez, Alvaro Ibañez
Crawford, Ken
Promper, Wolfgang
Jimenez, Manuel
Farras-Aloy, Silvia
Miro-Carretero, Juan
contents Tidal interactions between massive galaxies and their satellites are fundamental processes in a Universe with L-Cold Dark Matter cosmology, redistributing material into faint features that preserve records of past galactic interactions. While stellar streams in the Local Group impressively demonstrate satellite disruption, they do not constitute a statistically significant sample. Constructing a substantial catalog of stellar streams beyond the Local Group remains challenging due to the difficulties in obtaining deep, wide-field images of galaxies. Despite their potential to illuminate dark matter distribution and galaxy formation processes, stellar streams remain underutilized as cosmological probes. The Stellar Tidal Stream Survey (STSS) addresses this observational gap by leveraging amateur telescopes to obtain deep, scientific-grade images of galactic outskirts, capable of building a more statistically meaningful sample of stellar streams. Over the last decade, the STSS has acquired deep (up to surface brightness limit 28.3 mag/arcsec^2 in the r-band), wide-field images of 15 nearby Milky Way analog galaxies using a network of robotic amateur telescopes, avoiding the issues associated with "mosaicing" smaller images taken with a professional telescope. Our survey has revealed a diverse range of previously unreported faint features related to dwarf satellite accretion - including stellar streams, shells, and umbrella-like structures. We discover an ultra-diffuse galaxy (NGC150-UDG1), which shows hints of tidal tails. The STSS demonstrates the suitability of modern amateur telescopes to detect and study faint, diffuse structures in large fields around nearby spiral galaxies. Their economic and accessibility advantages enable larger samples with deep imaging, essential for testing galaxy formation models and constraining the properties of minor merger events in the local Universe.
format Preprint
id arxiv_https___arxiv_org_abs_2504_02071
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Stellar tidal streams around nearby spiral galaxies with deep imaging from amateur telescopes
Martinez-Delgado, David
Stein, Michael
Sakowska, Joanna D.
Weigelt, M. Maurice
Roman, Javier
Donatiello, Giuseppe
Roca-Fabrega, Santi
Schirmer, Mischa
Grebel, Eva K.
Saifollahi, Teymoor
Kanipe, Jeff
Gomez-Flechoso, M. Angeles
Akhlaghi, Mohammad
Javanmardi, Behnam
Wu, Gang
Eskandarlou, Sepideh
Bomans, Dominik J.
Henkel, Cristian
Block, Adam
Hanson, Mark
Schedler, Johannes
Teuwen, Karel
GaBany, R. Jay
Perez, Alvaro Ibañez
Crawford, Ken
Promper, Wolfgang
Jimenez, Manuel
Farras-Aloy, Silvia
Miro-Carretero, Juan
Astrophysics of Galaxies
Tidal interactions between massive galaxies and their satellites are fundamental processes in a Universe with L-Cold Dark Matter cosmology, redistributing material into faint features that preserve records of past galactic interactions. While stellar streams in the Local Group impressively demonstrate satellite disruption, they do not constitute a statistically significant sample. Constructing a substantial catalog of stellar streams beyond the Local Group remains challenging due to the difficulties in obtaining deep, wide-field images of galaxies. Despite their potential to illuminate dark matter distribution and galaxy formation processes, stellar streams remain underutilized as cosmological probes. The Stellar Tidal Stream Survey (STSS) addresses this observational gap by leveraging amateur telescopes to obtain deep, scientific-grade images of galactic outskirts, capable of building a more statistically meaningful sample of stellar streams. Over the last decade, the STSS has acquired deep (up to surface brightness limit 28.3 mag/arcsec^2 in the r-band), wide-field images of 15 nearby Milky Way analog galaxies using a network of robotic amateur telescopes, avoiding the issues associated with "mosaicing" smaller images taken with a professional telescope. Our survey has revealed a diverse range of previously unreported faint features related to dwarf satellite accretion - including stellar streams, shells, and umbrella-like structures. We discover an ultra-diffuse galaxy (NGC150-UDG1), which shows hints of tidal tails. The STSS demonstrates the suitability of modern amateur telescopes to detect and study faint, diffuse structures in large fields around nearby spiral galaxies. Their economic and accessibility advantages enable larger samples with deep imaging, essential for testing galaxy formation models and constraining the properties of minor merger events in the local Universe.
title Stellar tidal streams around nearby spiral galaxies with deep imaging from amateur telescopes
topic Astrophysics of Galaxies
url https://arxiv.org/abs/2504.02071