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20082022
most citedThe Carnegie-Irvine Galaxy Survey. I. Overview and Atlas of Optical Images

170 citations · 1.4k across the 31 of their papers we have counts for

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Showing 2017Show all

6 papers · 1 filter

astro-ph.GA2017★ 9 cited

Chemical abundances and ages of the bulge stars in APOGEE high-velocity peaks

Yingying Zhou, Juntai Shen, Chao Liu +17

A cold high-velocity (HV, 200 km/s) peak was first reported in several Galactic bulge fields based on the APOGEE commissioning observations. Both the existence and the natur…

astro-ph.GA2017★ 105 cited

Orbital decomposition of CALIFA spiral galaxies

Ling Zhu, Remco van den Bosch, Glenn van de Ven +9

Schwarzschild orbit-based dynamical models are widely used to uncover the internal dynamics of early-type galaxies and globular clusters. Here we present for the first time the Sch…

astro-ph.GA2017★ 40 cited

The Local Volume HI Survey: star formation properties

Jing Wang, Baerbel S. Koribalski, Tom H. Jarrett +12

We built a multi-wavelength dataset for galaxies from the Local Volume HI Survey (LVHIS), which comprises 82 galaxies. We also select a sub-sample of ten large galaxies for investi…

astro-ph.GA2017★ 71 cited

A parametric description of the 3D structure of the Galactic Bar/Bulge using the VVV survey

Iulia T. Simion, Vasily Belokurov, Mike Irwin +5

We study the structure of the inner Milky Way using the latest data release of the Vista Variables in Via Lactea (VVV) survey. The VVV is a deep near-infrared, multi-colour photome…

astro-ph.GA2017★ 45 cited

The Carnegie-Irvine Galaxy Survey. V. Statistical study of bars and buckled bars

Zhao-Yu Li, Luis C. Ho, Aaron J. Barth

Simulations have shown that bars are subject to a vertical buckling instability that transforms thin bars into boxy or peanut-shaped structures, but the physical conditions necessa…

astro-ph.GA2017★ 17 cited

The local spiral arm in the LAMOST-Gaia common stars?

Chao Liu, You-Gang Wang, Juntai Shen +7

Using the LAMOST-Gaia common stars, we demonstrate that the in-plane velocity field for the nearby young stars are significantly different from that for the old ones. For the young…