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Academic literature on the topic 'Starforce'

Author: Grafiati
Published: 4 June 2021
Last updated: 1 February 2022

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Journal articles on the topic "Starforce"

1

Guszejnov, Dávid, Michael Y. Grudić, Philip F. Hopkins, Stella S. R. Offner, and Claude-André Faucher-Giguère. "STARFORGE: the effects of protostellar outflows on the IMF." Monthly Notices of the Royal Astronomical Society 502, no. 3 (February 2, 2021): 3646–63. http://dx.doi.org/10.1093/mnras/stab278.

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ABSTRACT The initial mass function (IMF) of stars is a key quantity affecting almost every field of astrophysics, yet it remains unclear what physical mechanisms determine it. We present the first runs of the STAR FORmation in Gaseous Environments project, using a new numerical framework to follow the formation of individual stars in giant molecular clouds (GMCs) using the gizmo code. Our suite includes runs with increasingly complex physics, starting with isothermal ideal magnetohydrodynamics (MHD) and then adding non-isothermal thermodynamics and protostellar outflows. We show that without protostellar outflows the resulting stellar masses are an order of magnitude too high, similar to the result in the base isothermal MHD run. Outflows disrupt the accretion flow around the protostar, allowing gas to fragment and additional stars to form, thereby lowering the mean stellar mass to a value similar to that observed. The effect of jets upon global cloud evolution is most pronounced for lower mass GMCs and dense clumps, so while jets can disrupt low-mass clouds, they are unable to regulate star formation in massive GMCs, as they would turn an order unity fraction of the mass into stars before unbinding the cloud. Jets are also unable to stop the runaway accretion of massive stars, which could ultimately lead to the formation of stars with masses ${\gt}500\, \mathrm{M}_{\rm \odot }$. Although we find that the mass scale set by jets is insensitive to most cloud parameters (i.e. surface density, virial parameter), it is strongly dependent on the momentum loading of the jets (which is poorly constrained by observations) as well as the temperature of the parent cloud, which predicts slightly larger IMF variations than observed. We conclude that protostellar jets play a vital role in setting the mass scale of stars, but additional physics are necessary to reproduce the observed IMF.
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2

Markey, Carleen, Dávid Guszejnov, and Stella S. R. Offner. "Origins of Mass Segregation in Stellar Clusters within the STARFORGE Simulations." Research Notes of the AAS 4, no. 9 (September 23, 2020): 163. http://dx.doi.org/10.3847/2515-5172/abba78.

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Sari, Linna Oktaviana, and Aldi Kurniawan Batubara. "Impact of Different Topology on the Performance of IPSec VPN Multimedia Using CLSA." International Journal of Electrical, Energy and Power System Engineering 1, no. 2 (November 5, 2018): 20–25. http://dx.doi.org/10.31258/ijeepse.1.2.20-25.

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Due to multimedia application, network communication are expected to support multimedia traffic such as voice, video streaming and real time chat with a variety of Quality of Service (QoS) requirements. To support multimedia communications, it is desirable to use a network that meets QoS Parameter requirements. To deal with these challenges. In this study, VPN was designed with IPSec Tunneling. In designing VPN, the CLSA method is used. The network is composed of different topologies and uses OSPF as the routing protocol. Then multimedia traffic is passed on VPN networks to see the impact of different topologies on performance.The result show that theQuality of Service (QOS)in VPNobtained areaccording to ITU-T G.107 10 06/2015. The comparison of the average delay between the mesh and the star topology shows that the average delay in the mesh topology is 23% less than the starfor multimedia traffic. The comparison of the through put between the mesh topology and the star shows that the average throughputin the mesh topology is 68.8% betterthan the star for multimedia traffic. The comparison of the jitterbetween the mesh topology and the star shows that the average jitter in the star topology is 6%shorterthan the mesh for multimedia traffic.
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4

Grudić, Michael Y., Dávid Guszejnov, Philip F. Hopkins, Stella S. R. Offner, and Claude-André Faucher-Giguére. "STARFORGE: Toward a comprehensive numerical model of star cluster formation and feedback." Monthly Notices of the Royal Astronomical Society, May 17, 2021. http://dx.doi.org/10.1093/mnras/stab1347.

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Abstract We present STARFORGE (STAR FORmation in Gaseous Environments): a new numerical framework for 3D radiation MHD simulations of star formation that simultaneously follow the formation, accretion, evolution, and dynamics of individual stars in massive giant molecular clouds (GMCs) while accounting for stellar feedback, including jets, radiative heating and momentum, stellar winds, and supernovae. We use the GIZMO code with the MFM mesh-free Lagrangian MHD method, augmented with new algorithms for gravity, timestepping, sink particle formation and accretion, stellar dynamics, and feedback coupling. We survey a wide range of numerical parameters/prescriptions for sink formation and accretion and find very small variations in star formation history and the IMF (except for intentionally-unphysical variations). Modules for mass-injecting feedback (winds, SNe, and jets) inject new gas elements on-the-fly, eliminating the lack of resolution in diffuse feedback cavities otherwise inherent in Lagrangian methods. The treatment of radiation uses GIZMO’s radiative transfer solver to track 5 frequency bands (IR, optical, NUV, FUV, ionizing), coupling direct stellar emission and dust emission with gas heating and radiation pressure terms. We demonstrate accurate solutions for SNe, winds, and radiation in problems with known similarity solutions, and show that our jet module is robust to resolution and numerical details, and agrees well with previous AMR simulations. STARFORGE can scale up to massive (>105M⊙) GMCs on current supercomputers while predicting the stellar (≳ 0.1M⊙) range of the IMF, permitting simulations of both high- and low-mass cluster formation in a wide range of conditions.
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Books on the topic "Starforce"

1

Paulina, Ganucheau, Stern Sarah, Sawyer Christy, and Foxrobot Nikki, eds. Zodiac Starforce: Cries of the Fire Prince. Milwaukie, OR: Dark Horse Comics, 2018.

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2

Inc, Game Counselor. Game Counselor's Answer Book for Nintendo Players. Redmond, USA: Microsoft Pr, 1991.

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3

Comics, Marvel. Captain Marvel: Starforce. Marvel Worldwide, Incorporated, 2019.

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Behling, Steve. Captain Marvel: Starforce on the Rise. Marvel Press, 2019.

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illustrator, Ganucheau Paulina, Ganucheau Savanna illustrator, Sauvage Marguerite illustrator, Wada Kevin illustrator, Wyatt Jacob illustrator, and Tarr Babs illustrator, eds. Zodiac Starforce: By the power of Astra. 2016.

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6

Mega Man StarForce 2 Prima Official Game Guides. Prima Games, 2008.

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7

Starforce Hockey: The Greatest Players of Today and Tomorrow. Whitecap Books, 2000.

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8

Inc, Game Counsellor, ed. The Game Counsellor's answer book for Nintendo Game players: Hundredsof questions -and answers - about more than 250 popular Nintendo Games. Redmond, Washington: Microsoft Press, 1991.

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