activity
20052008
most citedVega is a rapidly rotating star

171 citations · 348 across the 6 of their papers we have counts for

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8 papers · 1 filter

astro-ph20082 cited

Solving the Imaging Problem with Coherently Integrated Multiwavelength Data

H. R. Schmitt, T. A. Pauls, J. T. Armstrong +7

Recovering images from optical interferometric observations is one of the major challenges in the field. Unlike the case of observations at radio wavelengths, in the optical the at…

astro-ph200849 cited

Constraining the Physical Parameters of the Circumstellar Disk of chi Ophiuchi

C. Tycner, C. E. Jones, T. A. A. Sigut +4

We present a numerical model describing a circularly symmetric gaseous disk around the Be star chi Ophiuchi. The model is constrained by long-baseline interferometric observations…

astro-ph200836 cited

A Parameter Study of Classical Be Star Disk Models Constrained by Optical Interferometry

C. E. Jones, C. Tycner, T. A. A. Sigut +2

We have computed theoretical models of circumstellar disks for the classical Be stars Dra, Psc, and Cyg. Models were constructed using a non-LTE radiative transf…

astro-ph200834 cited

Navy Prototype Optical Interferometer Imaging of Line Emission Regions of beta Lyrae Using Differential Phase Referencing

H. R. Schmitt, T. A. Pauls, C. Tycner +9

We present the results of an experiment to image the interacting binary star beta Lyrae with data from the Navy Prototype Optical Interferometer (NPOI), using a differential phase…

astro-ph2006171 cited

Vega is a rapidly rotating star

D. M. Peterson, C. A. Hummel, T. A. Pauls +8

Vega, the second brightest star in the northern hemisphere, serves as a primary spectral type standard. While its spectrum is dominated by broad hydrogen lines, the narrower lines…

astro-ph200656 cited

Constraining Disk Parameters of Be Stars using Narrowband H-alpha Interferometry with the NPOI

C. Tycner, G. C. Gilbreath, R. T. Zavala +7

Interferometric observations of two well-known Be stars, gamma Cas and phi Per, were collected and analyzed to determine the spatial characteristics of their circumstellar regions.…