The influence of different-concentrations 1-MCP on storing white celery

Guo, Zhenlong; Chen, Xiangning; Chang, Xiguang; Yang, Xiaofei; Guo, Y.H.; Zhong, Lianquan

doi:10.1201/b19126-85

Cited by 1 publication

(1 citation statement)

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“…Quilis & Trujillo (2012) estimated, using the Millennium Simulations, the expected fraction of massive galaxies with satellites with a mass ratio down to 1:10 and down to 1:100 within a sphere of R =100 kpc. They conducted their study exploring galaxies from z=2 to now using three different semi-analytical models (Bower et al 2006;DeLucia et al 2007;Guo et al 2011a). At z=0, the theoretical expectations suggested that the fraction of massive galaxies with at least a satellite down to 1:10 ranges from 0.3 to 0.4 and down to 1:100 from 0.6 to 0.7.…”

Section: Theorymentioning

confidence: 99%

The abundance of satellites depends strongly on the morphology of the host galaxy

Ruiz¹,

Trujillo

Mármol-Queraltó

2015

Mon. Not. R. Astron. Soc.

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Using the spectroscopic catalogue of the Sloan Digital Sky Survey Data Release 10, we have explored the abundance of satellites around a sample of 254 massive (10 11 < M ⋆ <2×10 11 M ⊙ ) local (z < 0.025) galaxies. We have divided our sample into four morphological groups (E, S0, Sa, Sb/c). We find that the number of satellites with M ⋆ 10 9 M ⊙ and R<300 kpc depends drastically on the morphology of the central galaxy. The average number of satellites per galaxy host (N Sat /N Host ) down to a mass ratio of 1:100 is: 4.5 ± 0.3 for E hosts, 2.6 ± 0.2 for S0, 1.5 ± 0.1 for Sa and 1.2 ± 0.2 for Sb/c. The amount of stellar mass enclosed by the satellites around massive E-type galaxies is a factor of 2, 4 and 5 larger than the mass in the satellites of S0, Sa and Sb/c-types, respectively. If these satellites would eventually infall into the host galaxies, for all the morphological types, the merger channel will be largely dominated by satellites with a mass ratio satellite-host µ >0.1. The fact that massive elliptical galaxies have a significant larger number of satellites than massive spirals could point out that elliptical galaxies inhabit heavier dark matter haloes than equally massive galaxies with later morphological types. If this hypothesis is correct, the dark matter haloes of late-type spiral galaxies are a factor of ∼2-3 more efficient on producing galaxies with the same stellar mass than those dark matter haloes of early-type galaxies.

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Section: Theorymentioning

confidence: 99%