A. Boselli
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View article: MAUVE-MUSE: A Star Formation-driven Outflow Caught in the Act of Quenching the Stripped Virgo Galaxy NGC 4064
MAUVE-MUSE: A Star Formation-driven Outflow Caught in the Act of Quenching the Stripped Virgo Galaxy NGC 4064 Open
The rapid quenching of satellite galaxies in dense environments is often attributed to environmental processes such as ram pressure stripping. However, stripping alone cannot fully account for the removal of dense, star-forming gas in many…
View article: PRIMAger General Observer programs: a π-sr Infrared Survey and other General Observer wide-field programs
PRIMAger General Observer programs: a π-sr Infrared Survey and other General Observer wide-field programs Open
The PRobe far-Infrared Mission for Astrophysics (PRIMA) is a cryogenically-cooled, far-infrared (far-IR) observatory expected to begin serving the astronomical community by early 2030. The mission features two advanced instruments: PRIMAge…
View article: Constraining Star Formation in M87 Using Deep Hubble Space Telescope UV Data
Constraining Star Formation in M87 Using Deep Hubble Space Telescope UV Data Open
We analyzed the deepest Hubble Space Telescope F275W ultraviolet (UV) imaging of M87 to obtain the most robust constraints on its star formation rate (SFR) and star formation history (SFH). After removing the galaxy continuum and globular …
View article: Unveiling the nature and fate of the almost-dark cloud AGC 226178 through H I mapping
Unveiling the nature and fate of the almost-dark cloud AGC 226178 through H I mapping Open
Context. The origin of extragalactic, almost dark H I clouds with extreme gas-to-stellar mass ratios remains poorly understood. Aims. We investigated the nature and fate of the almost dark cloud AGC 226178, projected within the Virgo clust…
View article: ALMA-JELLY. I. High Resolution CO(2–1) Observations of Ongoing Ram Pressure Stripping in NGC 4858 Reveal Asymmetrical Gas Tail Formation and Fallback
ALMA-JELLY. I. High Resolution CO(2–1) Observations of Ongoing Ram Pressure Stripping in NGC 4858 Reveal Asymmetrical Gas Tail Formation and Fallback Open
We present new CO(2–1) observations (resolution ∼1″ = 460 pc) of the Coma cluster jellyfish galaxy NGC 4858 obtained from the ALMA-JELLY large program. Analyzing this data alongside complimentary Subaru H α and Hubble Space Telescope (F600…
View article: Low surface brightness structures from annotated deep CFHT images: effects of the host galaxy’s properties and environment
Low surface brightness structures from annotated deep CFHT images: effects of the host galaxy’s properties and environment Open
Hierarchical galactic evolution models predict that mergers drive galaxy growth, producing low surface brightness (LSB) tidal features that trace galaxies’ late assembly. These faint structures encode information about past mergers and are…
View article: AVID: Formation and evolution of a coalesced major merger of late-type dwarf galaxies (VCC 479) on the outskirts of the Virgo cluster
AVID: Formation and evolution of a coalesced major merger of late-type dwarf galaxies (VCC 479) on the outskirts of the Virgo cluster Open
Context. Dwarf-dwarf galaxy mergers are among the least explored aspects of dwarf galaxy pre-processing as they fall into clusters. Aims. We present the first case study of a coalesced late-type dwarf major merger (VCC 479; stellar mass ∼ …
View article: Deep Galaxy Stellar Mass Functions As a Function of Star Formation Rate in the Virgo Cluster Environment
Deep Galaxy Stellar Mass Functions As a Function of Star Formation Rate in the Virgo Cluster Environment Open
We analyze deep ( M * ≳ 10 7 M ⊙ ) galaxy stellar mass functions (SMFs) of the Virgo cluster using stellar masses derived as part of the Next Generation Virgo Survey. The total SMF has a slope of , which is similar to or stee…
View article: <i>Euclid</i>: Early Release Observations of ram-pressure stripping in the Perseus cluster
<i>Euclid</i>: Early Release Observations of ram-pressure stripping in the Perseus cluster Open
Euclid is delivering optical and near-infrared imaging data over 14 000 deg 2 on the sky at spatial resolution and surface brightness levels that can be used to understand the morphological transformation of galaxies within groups and clus…
View article: Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Gas and dust in nearby galaxies
Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Gas and dust in nearby galaxies Open
Understanding the physical processes that regulate star formation and galaxy evolution are major areas of activity in modern astrophysics. Nearby galaxies offer unique opportunities to inspect interstellar medium (ISM), star formation (SF)…
View article: Deep galaxy stellar mass functions as a function of star formation rate in the Virgo cluster environment
Deep galaxy stellar mass functions as a function of star formation rate in the Virgo cluster environment Open
We analyze deep ($M_*\gtrsim10^7~{M}_{\odot}$) galaxy stellar mass functions (SMFs) of the Virgo cluster using stellar masses derived as part of the Next Generation Virgo Survey (NGVS). The total SMF has a slope of $α=-1.35^{+0.02}_{-0.02}…
View article: Star formation beyond galaxies: widespread in-situ formation of intra-cluster stars
Star formation beyond galaxies: widespread in-situ formation of intra-cluster stars Open
We study the fraction of the intra-cluster light (ICL) formed in-situ in the three most massive clusters of the TNG50 simulation, with virial masses . We find that a significant fraction of ICL stars ( - ) are born in-situ. T…
View article: ViCTORIA project: The LOFAR-MeerKAT view of active galactic nuclei in Virgo cluster early-type galaxies
ViCTORIA project: The LOFAR-MeerKAT view of active galactic nuclei in Virgo cluster early-type galaxies Open
The evolution of active galactic nuclei (AGNs) is closely connected to their host galaxies and surroundings. Via feedback processes, AGNs can counteract the cooling of the intracluster medium (ICM) and suppress star formation in their host…
View article: Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Gas and dust in nearby galaxies
Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Gas and dust in nearby galaxies Open
Understanding the physical processes that regulate star formation and galaxy evolution are major areas of activity in modern astrophysics. Nearby galaxies offer unique opportunities to inspect interstellar medium (ISM), star formation (SF…
View article: MAUVE: a 6 kpc bipolar outflow launched from NGC 4383, one of the most H <scp>i</scp>-rich galaxies in the Virgo cluster
MAUVE: a 6 kpc bipolar outflow launched from NGC 4383, one of the most H <span>i</span>-rich galaxies in the Virgo cluster Open
Stellar feedback-driven outflows are important regulators of the gas–star formation cycle. However, resolving outflow physics requires high-resolution observations that can only be achieved in very nearby galaxies, making suitable targets …
View article: Star formation beyond galaxies: widespread in-situ formation of intra-cluster stars
Star formation beyond galaxies: widespread in-situ formation of intra-cluster stars Open
We study the fraction of the intra-cluster light (ICL) formed in-situ in the three most massive clusters of the TNG50 simulation, with virial masses $\sim 10^{14}$ M$_{\odot}$. We find that a significant fraction of ICL stars ($8\%$-$28\%$…
View article: Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Gas and dust in nearby galaxies
Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Gas and dust in nearby galaxies Open
Understanding the physical processes that regulate star formation and galaxy evolution are major areas of activity in modern astrophysics. Nearby galaxies offer unique opportunities to inspect interstellar medium (ISM), star formation (SF)…
View article: ViCTORIA project: The LOFAR view of environmental effects in Virgo cluster star-forming galaxies
ViCTORIA project: The LOFAR view of environmental effects in Virgo cluster star-forming galaxies Open
Context. Environmental effects such as ram pressure stripping (RPS) shape the evolution of galaxies in dense regions. Aims. We used the nearby Virgo cluster as a laboratory to study the environmental effects on the nonthermal components of…
View article: The dynamical state of bars in cluster dwarf galaxies: the cases of NGC 4483 and NGC 4516
The dynamical state of bars in cluster dwarf galaxies: the cases of NGC 4483 and NGC 4516 Open
Dwarf barred galaxies are the perfect candidates for hosting slowly rotating bars. They are common in dense environments and have a relatively shallow potential well, making them prone to heating by interactions. When an interaction induce…
View article: The dynamical state of bars in cluster dwarf galaxies: The cases of NGC 4483 and NGC 4516
The dynamical state of bars in cluster dwarf galaxies: The cases of NGC 4483 and NGC 4516 Open
Dwarf barred galaxies are the perfect candidates for hosting slowly-rotating bars. They are common in dense environments and they have a relatively shallow potential well, making them prone to heating by interactions. When an interaction i…
View article: Nearby galaxies in the LOFAR Two-metre Sky Survey
Nearby galaxies in the LOFAR Two-metre Sky Survey Open
Context. To understand galaxy evolution, it is essential to measure star formation rates (SFRs) across cosmic time. Aims. The use of radio continuum emission as an extinction-free tracer of star formation necessitates a good understanding …
View article: ViCTORIA project: The LOFAR-view of environmental effects in Virgo Cluster star-forming galaxies
ViCTORIA project: The LOFAR-view of environmental effects in Virgo Cluster star-forming galaxies Open
Environmental effects such as ram-pressure stripping (RPS) shape the evolution of galaxies in dense regions. We use the nearby Virgo cluster as a laboratory to study environmental effects on the non-thermal components of star-forming galax…
View article: VERTICO and IllustrisTNG: The Spatially Resolved Effects of Environment on Galactic Gas
VERTICO and IllustrisTNG: The Spatially Resolved Effects of Environment on Galactic Gas Open
It has been shown in previous publications that the TNG100 simulation quantitatively reproduces the observed reduction in each of the total atomic and total molecular hydrogen gas for galaxies within massive halos, i.e., dense environments…
View article: VERTICO and IllustrisTNG: The spatially resolved effects of environment on galactic gas
VERTICO and IllustrisTNG: The spatially resolved effects of environment on galactic gas Open
It has been shown in previous publications that the TNG100 simulation quantitatively reproduces the observed reduction in each of the total atomic and total molecular hydrogen gas for galaxies within massive halos, i.e.~dense environments.…
View article: FAST-ASKAP Synergy: Quantifying Coexistent Tidal and Ram Pressure Strippings in the NGC 4636 Group
FAST-ASKAP Synergy: Quantifying Coexistent Tidal and Ram Pressure Strippings in the NGC 4636 Group Open
Combining new H i data from a synergetic survey of Australian Square Kilometre Array Pathfinder (ASKAP) Widefield ASKAP L -band Legacy All-sky Blind surveY and Five-hundred-meter Aperture Spherical radio Telescope with the Arecibo Legacy F…
View article: VERTICO. VII. Environmental Quenching Caused by the Suppression of Molecular Gas Content and Star Formation Efficiency in Virgo Cluster Galaxies
VERTICO. VII. Environmental Quenching Caused by the Suppression of Molecular Gas Content and Star Formation Efficiency in Virgo Cluster Galaxies Open
We study how environment regulates the star formation cycle of 33 Virgo Cluster satellite galaxies on 720 pc scales. We present the resolved star-forming main sequence for cluster galaxies, dividing the sample based on their global H i pro…
View article: VERTICO VII: Environmental quenching caused by suppression of molecular gas content and star formation efficiency in Virgo Cluster galaxies
VERTICO VII: Environmental quenching caused by suppression of molecular gas content and star formation efficiency in Virgo Cluster galaxies Open
We study how environment regulates the star formation cycle of 33 Virgo Cluster satellite galaxies on 720 parsec scales. We present the first resolved star-forming main sequence for cluster galaxies, dividing the sample based on their glob…
View article: Variation in optical and infrared properties of galaxies in relation to their surface brightness
Variation in optical and infrared properties of galaxies in relation to their surface brightness Open
Although it is now recognized that low surface brightness galaxies (LSBs) constitute a large fraction of the number density of galaxies, many of their properties are still poorly known. Based on only a few studies, LSBs are often considere…
View article: ViCTORIA project: MeerKAT HI observations of the ram pressure stripped galaxy NGC 4523
ViCTORIA project: MeerKAT HI observations of the ram pressure stripped galaxy NGC 4523 Open
We present the first results of a 21 cm HI line pilot observation carried out with MeerKAT in preparation for the ViCTORIA project, an untargeted survey of the Virgo galaxy cluster. The extraordinary quality of the data in terms of sensiti…
View article: VICTORIA project: The LOFAR HBA Virgo Cluster Survey
VICTORIA project: The LOFAR HBA Virgo Cluster Survey Open
Context. The Virgo cluster is the nearest ( d = 16.5 Mpc) massive ( M ≥ 10 14 M ⊙ ) galaxy cluster and is therefore a prime target for studying astrophysical processes in dense large-scale environments. In the radio band, we can probe the …