Zobrazeno 1 - 10
of 12 259
pro vyhledávání: '"Sills A"'
Autor:
Sills, Andrew V.
In 1986, composer Wendy Carlos introduced three unusual musical scales she called alpha, beta and gamma, equal temperament-inspired scales that de-emphasize the octave as the primary interval in favor of the major and minor thirds and the perfect fif
Externí odkaz:
http://arxiv.org/abs/2408.14551
Stellar clusters are critical constituents within galaxies: they are the result of highest-density star formation, and through their spatially and temporally correlated feedback they regulate their host galaxy evolution. We present a novel numerical
Externí odkaz:
http://arxiv.org/abs/2408.04694
Autor:
Nguyen, Michelle, Sills, Alison
We present a suite of binary evolution models with massive primaries (10 $\leq$ M$_1$ $\leq$ 40 M$_\odot$) and periods and mass ratios chosen such that the systems undergo non-conservative mass transfer while the primaries have helium cores. We track
Externí odkaz:
http://arxiv.org/abs/2405.05687
Autor:
Karam, Jeremy, Sills, Alison
We perform high resolution simulations of forming star clusters as they merge inside giant molecular clouds (GMCs) using hydrodynamics coupled to N-body dynamics to simultaneously model both the gas and stars. We zoom in to previously run GMC simulat
Externí odkaz:
http://arxiv.org/abs/2404.06348
Autor:
Schneider, Maxwell, McCarthy, Cody, Maxwell, Michael G., Pfeffer, Joshua, Schneider, Robert, Sills, Andrew V.
We detail the mathematical formulation of the line of "functional quantizer" modules developed by the Mathematics and Music Lab (MML) at Michigan Technological University, for the VCV Rack software modular synthesizer platform, which allow synthesize
Externí odkaz:
http://arxiv.org/abs/2404.04739
The presence or absence of star clusters in galaxies, and the properties of star cluster populations compared to their host galaxy properties, are important observables for validating models of cluster formation, galaxy formation, and galaxy assembly
Externí odkaz:
http://arxiv.org/abs/2307.14423
Massive star clusters are often used as tracers of galaxy formation and assembly. In order to do so, we must understand their properties at formation, and how those properties change with time, galactic environment, and galaxy assembly history. The t
Externí odkaz:
http://arxiv.org/abs/2306.17701
Autor:
Ferraro, Francesco R., Mucciarelli, Alessio, Lanzoni, Barbara, Pallanca, Cristina, Cadelano, Mario, Billi, Alex, Sills, Alison, Vesperini, Enrico, Dalessandro, Emanuele, Beccari, Giacomo, Monaco, Lorenzo, Mateo, Mario
Publikováno v:
Nature Communications 14, 2584 (2023)
Blue stragglers are anomalously luminous core hydrogen-burning stars formed through mass-transfer in binary/triple systems and stellar collisions. Their physical and evolutionary properties are largely unknown and unconstrained. Here we analyze 320 h
Externí odkaz:
http://arxiv.org/abs/2305.08478
Autor:
Karam, Jeremy, Sills, Alison
The formation of star clusters involves the growth of smaller, gas-rich subclusters through accretion of gas from the giant molecular cloud within which the subclusters are embedded. The two main accretion mechanisms responsible for this are accretio
Externí odkaz:
http://arxiv.org/abs/2303.11168
Autor:
Cournoyer-Cloutier, Claude, Sills, Alison, Harris, William E., Appel, Sabrina M., Lewis, Sean C., Polak, Brooke, Tran, Aaron, Wilhelm, Martijn J. C., Mac Low, Mordecai-Mark, McMillan, Stephen L. W., Zwart, Simon Portegies
We perform simulations of star cluster formation to investigate the morphological evolution of embedded star clusters in the earliest stages of their evolution. We conduct our simulations with Torch, which uses the AMUSE framework to couple state-of-
Externí odkaz:
http://arxiv.org/abs/2302.08536