output
20032025
most citedThe nature of the SDSS galaxies in various classes based on morphology, colour and spectral features -- I. Optical properties

30 citations

8 papers

astro-ph.GA2025

Conditions for Bar Formation in Bulgeless Disk Galaxies

Dajeong Jang, Woong-Tae Kim, Yun Hee Lee

While bars are commonly observed in disk galaxies, the precise conditions governing their formation remain incompletely understood. To investigate these conditions, we perform a su…

astro-ph.GA2025

Searching for Nearby Diffuse Dwarf Galaxies in the COSMOS Field

Dongdong Shi, XianZhong Zheng, Zhizheng Pan +5

It remains challenging to systematically survey nearby diffuse dwarf galaxies and address the formation mechanism of this population distinguishing from regular ones. We carry out…

astro-ph.GA2015★ 1 cited

Physical Properties of Tidal Features of Interacting Disk Galaxies: Three-dimensional Self-consistent Models

Sang Hoon Oh, Woong-Tae Kim, Hyung Mok Lee

Using self-consistent three-dimensional (3D) N-body simulations, we investigate the physical properties of non-axisymmetric features in a disk galaxy created by a tidal interaction…

physics.gen-ph2009

Dark Energy, Hyperbolic Cosecant Cardassian and Virial Collapse for Power-style Cardassian

Wen-Jie Tian

New work gathers in Chapter 6 and Chapter 7. Tthe Cardassian dynamical equations are introduced generally and logically under GF fluid scenario, together with the flowing process o…

astro-ph2008★ 30 cited

The nature of the SDSS galaxies in various classes based on morphology, colour and spectral features -- I. Optical properties

Joon Hyeop Lee, Myung Gyoon Lee, Changbom Park +1

We present a comprehensive study of the nature of the SDSS galaxies divided into various classes based on their morphology, colour, and spectral features. The SDSS galaxies are cla…

math.DG2007

Local rigidity in quaternionic hyperbolic space

Inkang Kim, Pierre Pansu

In this note, we study deformations of quaternionic hyperbolic lattices in larger quaternionic hyperbolic spaces and prove local rigidity results. On the other hand, surface groups…