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20032009
most citedUltra-cool dwarfs: new discoveries, proper motions, and improved spectral typing from SDSS and 2MASS photometric colors

53 citations · 76 across the 3 of their papers we have counts for

collaborators

5 papers

astro-ph.SR200923 cited

The masses of hot subdwarfs

X. Zhang, X. Chen, Z. Han

Masses are a fundamental parameter, but they are not well known for most hot subdwarfs. In general, the mass of a hot subdwarf is derived with asteroseismology or dynamical methods…

astro-ph.GA200953 cited

Ultra-cool dwarfs: new discoveries, proper motions, and improved spectral typing from SDSS and 2MASS photometric colors

Z. H. Zhang, R. S. Pokorny, H. R. A. Jones +6

Aims. We try to identify ultra-cool dwarfs from the seventh Data Release of the Sloan Digital Sky Survey (SDSS DR7) with SDSS i-z and r-z colors. We also obtain proper motion data…

astro-ph2008

The single degenerate channel for the progenitor of type Ia supernovae

Xiangcun Meng, Xuefei Chen, Zhanwen Han

We have carried out a detailed study of the single-degenerate channel for the progenitors of type Ia supernovae (SNe Ia). In the model, a carbon-oxygen white dwarf (CO WD) accretes…

astro-ph2004

Hot subdwarfs from the ESO Supernova Ia Progenitor Survey - I. Atmospheric parameters and cool companions of sdB stars

T. Lisker, U. Heber, R. Napiwotzki +4

We present the analysis of a high-resolution, high-quality sample of optical spectra for 76 subdwarf B (sdB) stars from the ESO Supernova Ia Progenitor Survey (SPY). Effective temp…

astro-ph2003

The single degenerate channel for the progenitors of type Ia supernovae

Zhanwen Han, Philipp Podsiadlowski

We have carried out a detailed study of one of the most popular evolutionary channels for the production of Type Ia supernova (SN Ia) progenitors, the semi-degenerate channel (CO+M…