Copertina

Distinguishing Ram Pressure from Tidal Interactions: the Size-Shape Difference (SSD) measure

Fuente: arXiv

Salvato in:

Dettagli Bibliografici
Autori principali:	Smith, Rory, Tonnesen, Stephanie, Kraljic, Katarina, Calderon-Castillo, Paula, Marasco, Antonino, Jaffe, Yara, Vulcani, Benedetta, Poggianti, Bianca M.
Natura:	Preprint
Pubblicazione:	2025
Soggetti:	Astrophysics of Galaxies
Accesso online:	Acceder al recurso
Tags:	Aggiungi Tag Nessun Tag, puoi essere il primo ad aggiungerne!!

Documenti analoghi

Distinguishing ram pressure from gravitational interactions: Applying the Size-Shape Difference method to real galaxies
di: Lassen, Augusto E., et al.
Pubblicazione: (2025)

Great Balls of Fire: Star Formation in Gas Clouds Accelerated by a Hot Wind
di: Tonnesen, Stephanie, et al.
Pubblicazione: (2026)

What goes around comes around: the fate of stars in stripped tails of gas
di: Akerman, Nina, et al.
Pubblicazione: (2025)

Gas Metallicity of Ram-Pressure Stripped Galaxies at Intermediate Redshift with MUSE Data
di: Khoram, Amir H., et al.
Pubblicazione: (2024)

The Competing Influence of Ram Pressure and Tidal Interaction in NGC 2276
di: Matijević, Luka, et al.
Pubblicazione: (2025)

With arms wide open: a VLT/MUSE view of the mechanisms driving unwinding spiral arms in cluster galaxies
di: Lassen, Augusto E., et al.
Pubblicazione: (2026)

Stripped and Enriched: The Role of Ram-Pressure in Shaping Chemical Enrichment of Galaxies at Intermediate Redshift
di: Khoram, Amir H., et al.
Pubblicazione: (2025)

The MUSE view of ram pressure stripped galaxies in clusters: the GASP sample
di: Poggianti, Bianca M., et al.
Pubblicazione: (2025)

The supersonic nature of jellyfish galaxies
di: Ignesti, Alessandro, et al.
Pubblicazione: (2026)

Constraining the duration of ram pressure stripping features in the optical from the direction of jellyfish galaxy tails
di: Salinas, Vicente, et al.
Pubblicazione: (2024)

Modelling the photometric and morphological evolution of disc galaxies in the cluster environment
di: Marasco, A., et al.
Pubblicazione: (2026)

Merging Galaxies in Isolated Environments II. Evolution of Star Formation and Accretion Activity during the Merging Process
di: Calderón-Castillo, Paula, et al.
Pubblicazione: (2024)

The interplay between Active Galactic Nuclei and Ram-pressure stripping: spatially resolved gas-phase abundances of stripped and undisturbed galaxies
di: Peluso, Giorgia, et al.
Pubblicazione: (2025)

The Evolution of the Spin Alignments of Dark Matter Halos in the Cosmic Web
di: Tobar, David, et al.
Pubblicazione: (2026)

Clump formation in ram-pressure stripped galaxies: evidence from mass function
di: Giunchi, Eric, et al.
Pubblicazione: (2025)

Unveiling Multiple Physical Processes on a Cluster Galaxy at z=0.3 Using JWST
di: Watson, Peter J., et al.
Pubblicazione: (2024)

Identification of ram pressure stripping features in galaxies using citizen science
di: Crossett, Jacob P., et al.
Pubblicazione: (2024)

Mechanisms Affecting Galaxies Nearby and Environmental Trends (MAGNET)
di: Vulcani, Benedetta, et al.
Pubblicazione: (2026)

Large Scale Structure and the Cosmic Web
di: Tojeiro, Rita, et al.
Pubblicazione: (2025)

Investigating the intracluster medium viscosity using the tails of GASP jellyfish galaxies
di: Ignesti, Alessandro, et al.
Pubblicazione: (2024)

Spatially resolved comparison of SFRs from UV and H$α$ in GASP gas-stripped galaxies
di: Tomicic, Neven, et al.
Pubblicazione: (2024)

SYMPHANY- SYnergy of Molecular PHase And Neutral hYdrogen in galaxies in A2626
di: Deb, Tirna, et al.
Pubblicazione: (2025)

The radial orbits of ram-pressure-stripped galaxies in clusters from the GASP survey
di: Biviano, A., et al.
Pubblicazione: (2024)

A cosmic degeneracy story: structure formation with warm dark matter and scale-dependent primordial non-Gaussianities
di: Stahl, Clément, et al.
Pubblicazione: (2025)

Two Channels of Metal-Rich Compact Stellar System Formation: Starbursts under High Ram Pressure versus Tidal Stripping
di: Bian, Yuan, et al.
Pubblicazione: (2024)

How galaxy properties vary with filament proximity in the SIMBA simulations
di: Bulichi, Teodora-Elena, et al.
Pubblicazione: (2023)

Large-scale geometry and topology of gas fields: Effects of AGN and stellar feedback
di: Schimd, Carlo, et al.
Pubblicazione: (2024)

New classification method for the dynamical state of galaxy clusters with a Gaussian mixture model
di: Kim, Hyowon, et al.
Pubblicazione: (2026)

Spatially resolved PAH$_{3.3}$ emission and stellar ages in ram pressure stripped clumps at $z\sim0.3$
di: Benotto, Pietro, et al.
Pubblicazione: (2025)

Dry ice baths as liquid nitrogen substitutes for physics demonstrations
di: Marasco, David, et al.
Pubblicazione: (2025)

Star formation at different stages of ram-pressure stripping as observed through far-ultraviolet imaging of 13 GASP galaxies
di: George, Koshy, et al.
Pubblicazione: (2025)

Anisotropy of Satellite Galaxies-I: Contrasting Correlations with Central Galaxy, Host Halo, and Large-Scale Filament Structures
di: Zhang, Zhuoming, et al.
Pubblicazione: (2026)

Geographical Variation in Body Size and Sexual Size Dimorphism ( SSD ) in the Epaulette Shark ( Hemiscyllium ocellatum )
di: Joel H. Gayford, et al.
Pubblicazione: (2026)

A 100 kpc Ram Pressure Tail Trailing the Group Galaxy NGC 2276
di: Roberts, I. D., et al.
Pubblicazione: (2024)

WLM: Dynamics of an isolated Dwarf Irregular Galaxy Under Ram Pressure in the Local Group
di: Kolhe, Neel, et al.
Pubblicazione: (2026)

The Role of Pre-Processing in Tidal Feature Formation within Galaxy Clusters
di: Chun, Kyungwon, et al.
Pubblicazione: (2025)

Not just PAH$_{3.3}$: why galaxies turn red in the Near-Infrared
di: Vulcani, Benedetta, et al.
Pubblicazione: (2024)

CARACTERIZAÇÃO MINERALÓGICA E BENEFICIAMENTO DAS BENTONITAS DA REGIÃO DE CUBATI E PEDRA LAVRADA-PB
di: D. A. Tonnesen
Pubblicazione: (2012)

Searching for correlations between satellite galaxy populations and the cold circumgalactic medium around TNG50 galaxies
di: Damle, Mitali, et al.
Pubblicazione: (2025)

Ram-Pressure Stripping Caught in Action in a Forming Cluster at $z \sim 2.5$
di: Xu, Ke, et al.
Pubblicazione: (2025)