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20022023
most citedThe Importance of Satellite Quenching for the Build-Up of the Red Sequence of Present Day Galaxies

458 citations · 5.6k across the 114 of their papers we have counts for

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Showing 2012Show all

6 papers · 1 filter

astro-ph.CO2012★ 52 cited

The dependence of tidal stripping efficiency on the satellite and host galaxy morphology

Jiang Chang, Andrea V. Maccio', Xi Kang

In this paper we study the tidal stripping process for satellite galaxies orbiting around a massive host galaxy, and focus on its dependence on the morphology of both satellite and…

astro-ph.SR2012★ 9 cited

Uncertainties in the calibrations of star formation rate

Fenghui Zhang, Lifang Li, Xiaoyu Kang +2

The calibrations of star formation rate (SFR) are prone to be affected by many factors, such as metallicity, initial mass function (IMF), evolutionary population synthesis (EPS) mo…

astro-ph.CO2012★ 42 cited

The effect of Warm Dark Matter on galaxy properties: constraints from the stellar mass function and the Tully-Fisher relation

Xi Kang, Andrea V. Macciò, Aaron A. Dutton

In this paper we combine high resolution N-body simulations with a semi analytical model of galaxy formation to study the effects of a possible Warm Dark Matter (WDM) component on…

astro-ph.CO2012★ 22 cited

The Evolution and Star Formation History of M33

Xiaoyu Kang, Ruixiang Chang, Jun Yin +4

We construct a parameterized model to explore the main properties of the star formation history of M33. We assume that the disk originates and grows by the primordial gas infall an…

astro-ph.CO2012★ 24 cited

Bulk flow of halos in ΛCDM simulation

Ming Li, Jun Pan, Liang Gao +10

Analysis of the Pangu N-body simulation validates that the bulk flow of halos follows a Maxwellian distribution which variance is consistent with the prediction of the linear theor…

astro-ph.CO2012★ 24 cited

Exploring Galaxy Formation Models and Cosmologies with Galaxy Clustering

X. Kang, M. Li, W. P. Lin +1

Using N-body simulations and galaxy formation models, we study the galaxy stellar mass correlation and the two-point auto-correlation. The simulations are run with cosmological par…