Derivation of the Binary Mass FunctionThe observational quantity f(m), the binary mass function, is derived.Eric Addison
STAR FORMATION: STATISTICAL MEASURE OF THE CORRELATION BETWEEN THE PRESTELLAR CORE MASS FUNCTION AND THE STELLAR INITIAL MASS FUNCTION We present a simple statistical analysis of recent numerical simulations exploring the correlation between the core mass function (CMF) obtained from the f... G Chabri...
In any case, the secondary star mass function is inconsistent with a Miller-ScaloYlike IMF unless the lower end is truncated below similar to 2-4 M-circle dot. In other words, massive stars preferentially have massive companions. The best-fitting models are described by a Salpeter or Miller...
The Initial Mass Function of the Massive Star-forming Region NGC 3603 from Near-Infrared Adaptive Optics Observations -CONICA at the VLT at ESO, we have successfully revealed the stellar population down to the subsolar mass range in the core of the starburst cluster... Y Harayama,F Eisenhauer...
We investigate how the properties of the merging binaries change with varying the SMBH mass, the slope of the initial mass function, the distributions of the binary orbital parameters, and the efficiency in energy dissipation in dissipative tides. We find that the fraction of merging massive ...
The main goal of our analysis is to test whether or not the observed companion mass ratio distribution (CMRD) as a function of primary star mass and star formation environment is consistent with having been drawn from the field star initial mass function (IMF). We consider samples of ...
The mass function of binary black hole merger depends on the angle of inclination of the orbital plane to the line of sight.()A.正确B.错误的答案是什么.用刷刷题APP,拍照搜索答疑.刷刷题(shuashuati.com)是专业的大学职业搜题找答案,刷题练习的工具.一键将文档
Sufficient velocity data are available to yield a preliminary orbit with a period of about 3.5 years and a mass function of 0.25 M/sub sun/. The excess infrared radiation is attributed to an unseen cool companion which has filled its Roche lobe and is losing mass. Some of this mass is ...
Globular ClustersMain Sequence StarsStellar SpectrophotometryCharge Coupled DevicesStellar LuminosityStellar MassPhotometry based on a mosaic of CCD images in B ... M Bolte - 《Astrophysical Journal Supplement》 被引量: 54发表: 1992年 An analytical description of the evolution of binary orbital-parameter...
This package implements a hierarchical bayesian framework for constraining the standard cosmological parameters (Hubble constant and Dark Matter density) and modified Gravitational Wave propagation parameters together with the Binary Black Hole (BBH) population parameters (mass function, merger rate density, ...