Zobrazeno 1 - 10
of 350
pro vyhledávání: '"Longmore, Steven N"'
Autor:
Kruijssen, J. M. Diederik, Valieva, Renata, Peluso, Kenneth, Emmons, Nicholas, Longmore, Steven N.
Publikováno v:
ADI 1, 20-27 (2024)
In decentralized systems, it is often necessary to select an 'active' subset of participants from the total participant pool, with the goal of satisfying computational limitations or optimizing resource efficiency. This selection can sometimes be mad
Externí odkaz:
http://arxiv.org/abs/2411.07302
Autor:
Battersby, Cara, Walker, Daniel L., Barnes, Ashley, Ginsburg, Adam, Lipman, Dani, Alboslani, Danya, Hatchfield, H Perry, Bally, John, Glover, Simon C. O., Henshaw, Jonathan D., Immer, Katharina, Klessen, Ralf S., Longmore, Steven N., Mills, Elisabeth A. C., Molinari, Sergio, Smith, Rowan, Sormani, Mattia C., Tress, Robin G., Zhang, Qizhou
The Central Molecular Zone (CMZ) is the largest reservoir of dense molecular gas in the Galaxy and is heavily obscured in the optical and near-IR. We present an overview of the far-IR dust continuum, where the molecular clouds are revealed, provided
Externí odkaz:
http://arxiv.org/abs/2410.17334
Autor:
Battersby, Cara, Walker, Daniel L., Barnes, Ashley, Ginsburg, Adam, Lipman, Dani, Alboslani, Danya, Hatchfield, H Perry, Bally, John, Glover, Simon C. O., Henshaw, Jonathan D., Immer, Katharina, Klessen, Ralf S., Longmore, Steven N., Mills, Elisabeth A. C., Molinari, Sergio, Smith, Rowan, Sormani, Mattia C., Tress, Robin G., Zhang, Qizhou
The Central Molecular Zone (CMZ) is the way station at the heart of our Milky Way Galaxy, connecting gas flowing in from Galactic scales with the central nucleus. Key open questions remain about its 3-D structure, star formation properties, and role
Externí odkaz:
http://arxiv.org/abs/2410.17332
Autor:
Lipman, Dani, Battersby, Cara, Walker, Daniel L., Sormani, Mattia C., Bally, John, Barnes, Ashley, Ginsburg, Adam, Glover, Simon C. O., Henshaw, Jonathan D., Hatchfield, H Perry, Immer, Katharina, Klessen, Ralf S., Longmore, Steven N., Mills, Elisabeth A. C., Smith, Rowan, Tress, R. G., Alboslani, Danya, Zhang, Qizhou
A comprehensive 3-D model of the central 300 pc of the Milky Way, the Central Molecular Zone (CMZ) is of fundamental importance in understanding energy cycles in galactic nuclei, since the 3-D structure influences the location and intensity of star f
Externí odkaz:
http://arxiv.org/abs/2410.17321
Autor:
Walker, Daniel L., Battersby, Cara, Lipman, Dani, Sormani, Mattia C., Ginsburg, Adam, Glover, Simon C. O., Henshaw, Jonathan D., Longmore, Steven N., Klessen, Ralf S., Immer, Katharina, Alboslani, Danya, Bally, John, Barnes, Ashley, Hatchfield, H Perry, Mills, Elisabeth A. C., Smith, Rowan, Tress, Robin G., Zhang, Qizhou
The Milky Way's Central Molecular Zone (CMZ) is the largest concentration of dense molecular gas in the Galaxy, the structure of which is shaped by the complex interplay between Galactic-scale dynamics and extreme physical conditions. Understanding t
Externí odkaz:
http://arxiv.org/abs/2410.17320
Autor:
Cotera, Angela S., Hankins, Matthew J., Bally, John, Barnes, Ashley T., Battersby, Cara D., Hatchfield, H Perry, Herter, Terry L., Lau, Ryan M., Longmore, Steven N., Mills, Elisabeth A. C., Morris, Mark R., Radomski, James T., Simpson, Janet P., Stephens, Zachary, Walker, Daniel L.
The central regions of the Milky Way constitute a unique laboratory for a wide swath of astrophysical studies, consequently the inner $\sim$400 pc has been the target of numerous large surveys at all accessible wavelengths. In this paper we present a
Externí odkaz:
http://arxiv.org/abs/2407.08054
Autor:
Schoedel, Rainer, Alberdi, Antxon, Jimenez-Serra, Izaskun, Yusef-Zadeh, Farhad, Gardini, Angela, Kramer, Michael, Torres, Miguel Perez, Morris, Mark R., Forbrich, Jan, Ingallinera, Adriano, Nogueras-Lara, Francisco, Henshaw, Jonathan D., Longmore, Steven N., Moldon, Javier, Heywood, Ian, Rammala, Isabella, Montenegro, Lourdes Verdes, Exposito, Susana Sanchez
With its extreme density of stars and stellar remnants, dense young massive clusters, high specific star formation rate, intense radiation field, high magnetic field strength, and properties of the interstellar medium that resemble those in high reds
Externí odkaz:
http://arxiv.org/abs/2406.04022
Autor:
Kruijssen, J. M. Diederik, Chevance, Mélanie, Longmore, Steven N., Ginsburg, Adam, Ramambason, Lise, Romanelli, Andrea
Recent observations have demonstrated that giant molecular clouds (GMCs) are short-lived entities, surviving for the order of a dynamical time before turning a few percent of their mass into stars and dispersing, leaving behind an isolated young stel
Externí odkaz:
http://arxiv.org/abs/2404.14495
Autor:
Ginsburg, Adam, Bally, John, Barnes, Ashley T., Battersby, Cara, Budaiev, Nazar, Butterfield, Natalie O., Caselli, Paola, Colzi, Laura, Dutkowska, Katarzyna M., García, Pablo, Gramze, Savannah, Henshaw, Jonathan D., Hu, Yue, Jeff, Desmond, Jiménez-Serra, Izaskun, Kauffmann, Jens, Klessen, Ralf S., Levesque, Emily M., Longmore, Steven N., Lu, Xing, Mills, Elisabeth A. C., Morris, Mark R., Nogueras-Lara, Francisco, Oka, Tomoharu, Pineda, Jaime E., Pillai, Thushara G. S., Rivilla, Víctor M., Sánchez-Monge, Álvaro, Santa-Maria, Miriam G., Smith, Howard A., Sofue, Yoshiaki, Sormani, Mattia C., Tremblay, Grant R., Vermariën, Gijs, Vikhlinin, Alexey, Viti, Serena, Walker, Dan, Wang, Q. Daniel, Xu, Fengwei, Zhang, Qizhou
A compact source, G0.02467-0.0727, was detected in ALMA \threemm observations in continuum and very broad line emission. The continuum emission has a spectral index $\alpha\approx3.3$, suggesting that the emission is from dust. The line emission is d
Externí odkaz:
http://arxiv.org/abs/2404.07808
Autor:
Hatchfield, H Perry, Battersby, Cara, Barnes, Ashley T., Butterfield, Natalie, Ginsburg, Adam, Henshaw, Jonathan D., Longmore, Steven N., Lu, Xing, Svoboda, Brian, Walker, Daniel, Callanan, Daniel, Mills, Elisabeth A. C., Ho, Luis C., Kauffmann, Jens, Kruijssen, J. M. Diederik, Ott, Jürgen, Pillai, Thushara, Zhang, Qizhou
In this work, we constrain the star-forming properties of all possible sites of incipient high-mass star formation in the Milky Way's Galactic Center. We identify dense structures using the CMZoom 1.3mm dust continuum catalog of objects with typical
Externí odkaz:
http://arxiv.org/abs/2312.09284