activity
20042008
most citedRevealing the Nature of Algol Disks through Optical and UV Spectroscopy, Synthetic Spectra, and Tomography of TT Hydrae

41 citations · 83 across the 5 of their papers we have counts for

collaborators

8 papers

astro-ph2008

Report IAU Comm. 42, Close Binary Stars

Slavek M. Rucinski, Ignasi Ribas, Colin D. Scarfe +5

Brief summaries are given about (1) close binary research from the perspective of the Bibliography of Close Binaries, (2) low-mass binaries and model discrepancies, (3) W UMa-type…

astro-ph200819 cited

Three-Dimensional Doppler Images of the Disk-like and Stream-like States of U Coronae Borealis

Michail Agafonov, Olga Sharova, Mercedes Richards

The 3D Radioastronomical Approach to Doppler tomography has been used to study the H emission sources in U Coronae Borealis. These 3D tomograms provide greater resolution than t…

astro-ph200641 cited

Revealing the Nature of Algol Disks through Optical and UV Spectroscopy, Synthetic Spectra, and Tomography of TT Hydrae

Brendan Miller, Jan Budaj, Mercedes Richards +2

We have developed a systematic procedure to study the disks in Algol-type binaries using spectroscopic analysis, synthetic spectra, and tomography. We analyzed 119 H-alpha spectra…

astro-ph20064 cited

Long-term Variability in the Length of the Solar Cycle

Michael L. Rogers, Mercedes T. Richards, Donald St. P. Richards

Detailed models of the solar cycle require information about the starting time and rise time as well as the shape and amplitude of the cycle. However, none of these models includes…

astro-ph200619 cited

Nova V4743 Sagittarii 2002: An Intermediate Polar Candidate

Tae W. Kang, Alon Retter, Alex Liu +1

We present the results of 11 nights of CCD unfiltered photometry of V4743 Sgr (Nova Sgr 2002 # 3) from 2003 and 2005. We find two periods of 0.2799 d ~ 6.7 h and 0.01642 d ~ 24 min…

astro-ph2005

Detection of orbital and superhump periods in Nova V2574 Ophiuchi (2004)

Tae W. Kang, Alon Retter, Alex Liu +1

We present the results of 37 nights of CCD unfiltered photometry of nova V2574 Oph (2004) from 2004 and 2005. We find two periods of 0.14164 d (~3.40 h) and 0.14773 d (~3.55 h) in…