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20102026
most citedBinary Cepheids: Separations and Mass Ratios in Binaries

53 citations · 113 across the 8 of their papers we have counts for

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astro-ph.SR2020

Hubble Space Telescope Snapshot Survey for Resolved Companions of Galactic Cepheids: Final Results

Nancy Remage Evans, H. Moritz Guenther, Howard E. Bond +13

Cepheids in multiple systems provide information on the outcome of the formation of massive stars. They can also lead to exotic end-stage objects. This study concludes our survey o…

astro-ph.SR2018★ 16 cited

The Orbit of the Close Companion of Polaris: Hubble Space Telescope Imaging 2007 to 2014

Nancy Remage Evans, Margarita Karovska, Howard E. Bond +6

As part of a program to determine dynamical masses of Cepheids, we have imaged the nearest and brightest Cepheid, Polaris, with the Hubble Space Telescope Wide Field Planetary Came…

astro-ph.SR2016★ 14 cited

Hubble Space Telescope: Snapshot Survey for Resolved Companions of Galactic Cepheids

Nancy Remage Evans, Howard E. Bond, Gail H. Schaefer +4

We have conducted an imaging survey with the Hubble Space Telescope Wide Field Camera~3 (WFC3) of 70 Galactic Cepheids, typically within 1~kpc, with the aim of finding resolved phy…

astro-ph.SR2016★ 15 cited

Resolved Companions of Cepheids: Testing the Candidates with X-Ray Observations

Nancy Remage Evans, Ignazio Pillitteri, Scott Wolk +7

We have made {\it XMM-Newton\/} observations of 14 Galactic Cepheids that have candidate resolved (5$\arcsec$) companion stars based on our earlier {\it HST\/} WFC3 imaging s…

astro-ph.SR2014★ 5 cited

X-ray Detection of the Cluster Containing the Cepheid S Mus

Nancy Remage Evans, Ignazio Pillitteri, Scott J. Wolk +7

The galactic Cepheid S Muscae has recently been added to the important list of Cepheids linked to open clusters, in this case the sparse young cluster ASCC 69. Low-mass members of…

astro-ph.SR2013★ 53 cited

Binary Cepheids: Separations and Mass Ratios in Binaries

Nancy Remage Evans, Howard E. Bond, Gail H. Schaefer +3

Deriving the distribution of binary parameters for a particular class of stars over the full range of orbital separations usually requires the combination of results from many diff…