Comparing the $M_{gas}-N_{yso}$ Relation inside a Giant Molecular Cloud
Fuente:
arXiv
Saved in:
| Main Authors: | Román-Zúñiga, Carlos G., Palau, Aina, Ballesteros-Paredes, Javier, Zamora-Avilés, Manuel, Peltonen, Joshua, Gutiérrez-Davila, Karla |
|---|---|
| Format: | Preprint |
| Published: |
2026
|
| Subjects: | |
| Online Access: | |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
Gravity or turbulence? VI. The physics behind the Kennicutt-Schmidt relations
by: Ballesteros-Paredes, Javier, et al.
Published: (2024)
by: Ballesteros-Paredes, Javier, et al.
Published: (2024)
The sonic scale does not determine the core separation in turbulent molecular clouds
by: Manuel, Zamora-Aviles, et al.
Published: (2025)
by: Manuel, Zamora-Aviles, et al.
Published: (2025)
Pressure Regulated Formation of Molecular Clouds and Stars: The case of the Milky Way
by: Franco, José, et al.
Published: (2025)
by: Franco, José, et al.
Published: (2025)
Synthetic polarization observations of magnetized pillars in HII regions: The limitations of the Davis-Chandrasekhar-Fermi method
by: Hernández-Cruz, Luis Andrés, et al.
Published: (2025)
by: Hernández-Cruz, Luis Andrés, et al.
Published: (2025)
Gravity or turbulence? VII. The Schmidt-Kennicutt law, the star formation efficiency, and the mass density of clusters from gravitational collapse rather than turbulent support
by: Zamora-Aviles, Manuel, et al.
Published: (2024)
by: Zamora-Aviles, Manuel, et al.
Published: (2024)
Dynamical heating of newborn stars driven by accretion-induced orbital tightening
by: Camacho, Vianey, et al.
Published: (2025)
by: Camacho, Vianey, et al.
Published: (2025)
Clusters, Clouds, and Correlations: Relating Young Clusters to Giant Molecular Clouds in M33 and M31
by: Peltonen, J., et al.
Published: (2023)
by: Peltonen, J., et al.
Published: (2023)
The Turbulent Support (TS) and Global Hierarchical Collapse (GHC) models for molecular clouds compared. Differences, convergence, and myths
by: Vázquez-Semadeni, Enrique, et al.
Published: (2024)
by: Vázquez-Semadeni, Enrique, et al.
Published: (2024)
Unveiling two expanding stellar groups formed through violent relaxation in The Lagoon Nebula Cluster
by: Bonilla-Barroso, A., et al.
Published: (2024)
by: Bonilla-Barroso, A., et al.
Published: (2024)
Can radial temperature profiles be inferred using NH3 (1, 1) and (2, 2) observations?
by: Estalella, Robert, et al.
Published: (2024)
by: Estalella, Robert, et al.
Published: (2024)
On the relation between magnetic field strength and gas density in the interstellar medium. II. Density uncertainties and diffuse gas constraints
by: Whitworth, David, et al.
Published: (2026)
by: Whitworth, David, et al.
Published: (2026)
Thermodynamics of Giant Molecular Clouds: The Effects of Dust Grain Size
by: Soliman, Nadine H., et al.
Published: (2024)
by: Soliman, Nadine H., et al.
Published: (2024)
Hierarchical Structure and Self-gravity in the Maddalena Giant Molecular Cloud
by: Shen, Renjie, et al.
Published: (2024)
by: Shen, Renjie, et al.
Published: (2024)
Absence of High-mass Prestellar Cores in the Orion Giant Molecular Cloud
by: Jiao, Wenyu, et al.
Published: (2024)
by: Jiao, Wenyu, et al.
Published: (2024)
Resolved Dust Emission and CO Isotopologues in Giant Molecular Clouds of the Andromeda Galaxy
by: Bosomworth, Chloe, et al.
Published: (2026)
by: Bosomworth, Chloe, et al.
Published: (2026)
Observations of pre- and proto-brown dwarfs in nearby clouds: paving the way to further constraining theories of brown dwarf formation
by: Palau, Aina, et al.
Published: (2024)
by: Palau, Aina, et al.
Published: (2024)
The Magnetic Keys to Massive Star Formation: The Western $η$ Carinae Giant Molecular Cloud
by: Barnes, Peter J., et al.
Published: (2025)
by: Barnes, Peter J., et al.
Published: (2025)
Deep Andromeda JCMT-SCUBA2 Observations. The Submillimeter Maps and Giant Molecular Clouds
by: Jiao, Sihan, et al.
Published: (2025)
by: Jiao, Sihan, et al.
Published: (2025)
Giant Molecular Clouds in RCW 106 (G333): Galactic Mini-starbursts and Massive Star Formation Induced by Supersonic Cloud-Cloud Collisions
by: Kohno, Mikito, et al.
Published: (2025)
by: Kohno, Mikito, et al.
Published: (2025)
Dense gas tracers in and between spiral arms: from Giant Molecular Filaments to star-forming clumps
by: Feher, O., et al.
Published: (2025)
by: Feher, O., et al.
Published: (2025)
Kinematic study of the Orion Complex: Analysing the young stellar clusters from big and small structures
by: Sánchez-Sanjuán, Sergio, et al.
Published: (2024)
by: Sánchez-Sanjuán, Sergio, et al.
Published: (2024)
Revisiting the Velocity Dispersion-Size Relation in Molecular Cloud Structures
by: Feng, Haoran, et al.
Published: (2024)
by: Feng, Haoran, et al.
Published: (2024)
On the Flux-Intensity Relation of Molecular Clouds
by: Yan, Qing-Zeng, et al.
Published: (2024)
by: Yan, Qing-Zeng, et al.
Published: (2024)
Random gas motions inside sub-parsec scale supercritical filaments
by: Zhang, Chao, et al.
Published: (2026)
by: Zhang, Chao, et al.
Published: (2026)
A New Cloud-Cloud Collision Source N68 toward the G35 Molecular Cloud Complex
by: Chen, En, et al.
Published: (2026)
by: Chen, En, et al.
Published: (2026)
Discovery of a Giant Molecular Cloud at the Midpoint of the Galactic Bar Dust Lanes: M4.7-0.8
by: Butterfield, Natalie, et al.
Published: (2025)
by: Butterfield, Natalie, et al.
Published: (2025)
Near-Ultraviolet Radiation toward Molecular Cloud N4 in W 50/SS 433: Evidence for Direct Interaction of the Jet with Molecular Cloud
by: Yamamoto, H., et al.
Published: (2024)
by: Yamamoto, H., et al.
Published: (2024)
A framework for modeling the evolution of young stellar objects
by: Richardson, Theo, et al.
Published: (2025)
by: Richardson, Theo, et al.
Published: (2025)
ACA CO(J=2-1) Mapping of the Nearest Spiral Galaxy M33. II. Exploring the Evolution of Giant Molecular Clouds
by: Konishi, Ayu, et al.
Published: (2024)
by: Konishi, Ayu, et al.
Published: (2024)
A Kinematic Analysis of the Giant Molecular Complex W3; Possible Evidence for Cloud-Cloud Collisions that Triggered OB Star Clusters in W3 Main and W3(OH)
by: Yamada, R. I., et al.
Published: (2021)
by: Yamada, R. I., et al.
Published: (2021)
Estimating the Luminosities of Protostars with Limited Infrared Photometry
by: Dunham, Michael M., et al.
Published: (2026)
by: Dunham, Michael M., et al.
Published: (2026)
The Molecular Clouds of M31
by: Lada, Charles J., et al.
Published: (2024)
by: Lada, Charles J., et al.
Published: (2024)
Connecting Star Formation in the Milky Way and Nearby Galaxies. I. Comparability of Molecular Cloud Physical Properties
by: Zhou, J. W., et al.
Published: (2025)
by: Zhou, J. W., et al.
Published: (2025)
Peculiar galaxies I: A Catalog of Polar-Ring Galaxies from the TNG50 Simulation
by: López-Castillo, Josué G., et al.
Published: (2025)
by: López-Castillo, Josué G., et al.
Published: (2025)
ALMA Observations of Molecular Complexity in the Large Magellanic Cloud: Probing the Star-forming Region N160
by: Broadmeadow, Amanda, et al.
Published: (2025)
by: Broadmeadow, Amanda, et al.
Published: (2025)
A VLA search for compact radio sources in the explosive molecular outflows DR 21 and G5.89
by: Yanza, Vanessa, et al.
Published: (2025)
by: Yanza, Vanessa, et al.
Published: (2025)
Cloud-Scale Molecular Gas Properties of the Antennae Merger: A Comparative Study with PHANGS-ALMA Galaxies and NGC 3256
by: Brunetti, Nathan, et al.
Published: (2024)
by: Brunetti, Nathan, et al.
Published: (2024)
The Molecular Cloud Lifecycle II: Formation and Destruction of Molecular Clouds Diagnosed via H$_2$ Fluorescent Emission Emission
by: Burkhart, Blakesley, et al.
Published: (2024)
by: Burkhart, Blakesley, et al.
Published: (2024)
Characterizing the 3D Structure of Molecular Cloud Envelopes in the "Cloud Factory" Simulations
by: Mullens, Elijah, et al.
Published: (2024)
by: Mullens, Elijah, et al.
Published: (2024)
The Giant Molecular Cloud G148.24+00.41: Gas Properties, Kinematics, and Cluster Formation at the Nexus of Filamentary Flows
by: Rawat, Vineet, et al.
Published: (2024)
by: Rawat, Vineet, et al.
Published: (2024)
Similar Items
-
Gravity or turbulence? VI. The physics behind the Kennicutt-Schmidt relations
by: Ballesteros-Paredes, Javier, et al.
Published: (2024) -
The sonic scale does not determine the core separation in turbulent molecular clouds
by: Manuel, Zamora-Aviles, et al.
Published: (2025) -
Pressure Regulated Formation of Molecular Clouds and Stars: The case of the Milky Way
by: Franco, José, et al.
Published: (2025) -
Synthetic polarization observations of magnetized pillars in HII regions: The limitations of the Davis-Chandrasekhar-Fermi method
by: Hernández-Cruz, Luis Andrés, et al.
Published: (2025) -
Gravity or turbulence? VII. The Schmidt-Kennicutt law, the star formation efficiency, and the mass density of clusters from gravitational collapse rather than turbulent support
by: Zamora-Aviles, Manuel, et al.
Published: (2024)