Imagen de Portada

The mmax-Mecl relation in the LEGUS clusters

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Zinnkann, Marie, Jerabkova, Tereza, Yan, Zhiqiang, Kroupa, Pavel, Ostermann, Yannik, Gjergo, Eda, Zonoozi, Akram Hasani, Haghi, Hosein, Pflamm-Altenburg, Jan
Formato:	Preprint
Publicado:	2026
Materias:	Astrophysics of Galaxies
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

The effect of the environment-dependent stellar initial mass function on the baryonic Tully Fisher relation
por: Zonoozi, Akram Hasani, et al.
Publicado: (2025)

The effect of the environment-dependent stellar initial mass function on the photometric properties of star-forming galaxies
por: Haslbauer, Moritz, et al.
Publicado: (2024)

Stellar population synthesis models with a physically varying IMF
por: Zonoozi, Akram Hasani, et al.
Publicado: (2025)

Are the ONC, Pleiades, and Hyades snapshots of the same embedded cluster?
por: Safaei, Ghasem, et al.
Publicado: (2025)

Has the Palomar 14 globular cluster been captured by the Milky Way?
por: Zonoozi, Akram Hasani, et al.
Publicado: (2024)

Origin of open clusters revealed by the evolution of the m_max$-$M_ecl relation
por: Zhou, J. W., et al.
Publicado: (2026)

Massive Star Formation at Supersolar Metallicities: Constraints on the Initial Mass Function
por: Gjergo, Eda, et al.
Publicado: (2025)

The initial mass function of stars
por: Kroupa, Pavel, et al.
Publicado: (2024)

Dark Star Clusters or Ultra-Faint Dwarf galaxies? Revisiting UMa3/U1
por: Rostami-Shirazi, Ali, et al.
Publicado: (2025)

The impact of a top-heavy IMF on the formation and evolution of dark star clusters
por: Shirazi, Ali Rostami, et al.
Publicado: (2024)

Mass segregation and velocity dispersion as evidence for a dark star cluster
por: Wu, Wenjie, et al.
Publicado: (2024)

Semi-supervised classification of stars, galaxies and quasars using K-means and random-forest approaches
por: Asadi, Vahid, et al.
Publicado: (2025)

Machine Learning vs. Spectral Energy Distribution Fitting: A Comparative Analysis of Accuracy in Stellar Mass Estimation
por: Asadi, Vahid, et al.
Publicado: (2025)

Open star clusters and their asymmetrical tidal tails
por: Kroupa, Pavel, et al.
Publicado: (2024)

Revisiting the missing mass problem in MOND for nearby galaxy clusters
por: Zhang, Dong, et al.
Publicado: (2026)

The p-Laplacian as a Framework for Generalizing Newtonian Gravity and MoND
por: Scherer, D., et al.
Publicado: (2025)

Universal depletion of metal-poor globular clusters in inner galaxy regions: Fossil record of black hole retention
por: Rostami-Shirazi, Ali, et al.
Publicado: (2025)

Origin of the metal-rich vs. metal-poor globular clusters dichotomies in the Milky Way: A sign of low black hole natal kicks
por: Rostami-Shirazi, Ali, et al.
Publicado: (2024)

The Variation of the Galaxy-Wide IMF for Low-Mass Stars: Modeling and Observational Insights
por: Yan, Zhiqiang, et al.
Publicado: (2024)

The Impact of Early Massive Galaxy Formation on the Cosmic Microwave Background
por: Gjergo, Eda, et al.
Publicado: (2025)

The formation and evolution of dark star clusters II: The impact of primordial mass segregation
por: Ghasemi, S. Mojtaba, et al.
Publicado: (2024)

Self-regulated galaxy evolution within a self-consistently varying galaxy-wide IMF
por: Hof, Lukas, et al.
Publicado: (2026)

Asymmetry of the tidal tails of open star clusters in direct N-body integrations in Milgrom-law dynamics
por: Pflamm-Altenburg, J.
Publicado: (2024)

The spin, expansion and contraction of open star clusters
por: Jadhav, Vikrant V., et al.
Publicado: (2024)

Effects of physical conditions on the stellar initial mass function: The low-metallicity star-forming region Sh 2-209
por: Zinnkann, Marie, et al.
Publicado: (2024)

Origin of High Dark Remnant Fractions in Milky Way Globular Clusters: The Crucial Role of Initial Black Hole Retention
por: Rostami-Shirazi, Ali, et al.
Publicado: (2025)

The Initial Mass Function as the Equilibrium State of a Variational Process: why the IMF cannot be sampled stochastically
por: Gjergo, Eda, et al.
Publicado: (2026)

Numerical solutions of the complete two-body system in QUMOND
por: Pflamm-Altenburg, J.
Publicado: (2025)

Machine Learning Classification of COSMOS2020 Galaxies: Quiescent vs. Star-Forming
por: Asadi, Vahid, et al.
Publicado: (2025)

Leveraging Machine Learning for Accurate and Fast Stellar Mass Estimation of Galaxies
por: Asadi, Vahid, et al.
Publicado: (2025)

Failed supernova explosions increase the duration of star formation in globular clusters
por: Wirth, Henriette, et al.
Publicado: (2024)

The evolution of the mass--radius relation of expanding very young star clusters
por: Zhou, Jian-Wen, et al.
Publicado: (2024)

Scaling relations of early-type galaxies in MOND
por: Eappen, Robin, et al.
Publicado: (2025)

The post-gas expulsion coalescence of embedded clusters as an origin of open clusters
por: Zhou, J. W., et al.
Publicado: (2025)

Are binary-star populations regionally different? --in memory of Sverre Aarseth--
por: Kroupa, Pavel
Publicado: (2025)

Self-similar cluster structures in massive star-forming regions: Isolated evolution from clumps to embedded clusters
por: Zhou, J. W., et al.
Publicado: (2024)

Intermediate-mass black hole incubators. Gas accretion onto stellar black hole clusters in galactic central molecular zones
por: Haas, Jaroslav, et al.
Publicado: (2026)

Tidal tails of nearby open clusters I. Mapping with Gaia DR3
por: Risbud, Dhanraj, et al.
Publicado: (2025)

The currently observed clumps cannot be the "direct" precursors of the currently observed open clusters
por: Zhou, J. W., et al.
Publicado: (2024)

The masses of open star clusters and their tidal tails and the stellar initial mass function
por: Wirth, Henriette, et al.
Publicado: (2024)