J. M. Nemec
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View article: Double-Mode RR Lyrae Stars Observed by K2: Analysis of High-Precision Kepler Photometry
Double-Mode RR Lyrae Stars Observed by K2: Analysis of High-Precision Kepler Photometry Open
The results of a Fourier analysis of high-precision Kepler photometry of 75 double-mode RR~Lyrae (RRd) stars observed during NASA's K2 Mission (2014-18) are presented. Seventy-two of the stars are `classical' RRd (cRRd) stars lying along a…
View article: Double-mode RR Lyrae stars observed by <i>K2</i>: analysis of high-precision <i>Kepler</i> photometry
Double-mode RR Lyrae stars observed by <i>K2</i>: analysis of high-precision <i>Kepler</i> photometry Open
The results of a Fourier analysis of high-precision Kepler photometry of 75 double-mode RR Lyrae (RRd) stars observed during NASA’s K2 Mission (2014-18) are presented. Seventy-two of the stars are ‘classical’ RRd (cRRd) stars lying along a…
View article: First Results on RR Lyrae Stars with the TESS Space Telescope: Untangling the Connections between Mode Content, Colors, and Distances
First Results on RR Lyrae Stars with the TESS Space Telescope: Untangling the Connections between Mode Content, Colors, and Distances Open
The Transiting Exoplanet Survey Satellite (TESS) space telescope is collecting continuous, high-precision optical photometry of stars throughout the sky, including thousands of RR Lyrae stars. In this paper, we present results for an initi…
View article: The first view of δ Scuti and γ Doradus stars with the TESS mission
The first view of δ Scuti and γ Doradus stars with the TESS mission Open
© 2019 The Author(s) We present the first asteroseismic results for δ Scuti and γ Doradus stars observed in Sectors 1 and 2 of the TESS mission. We utilize the 2-min cadence TESS data for a sample of 117 stars to classify their behaviour r…
View article: Four ‘Peculiar’ RRd stars observed by <i>K2</i>
Four ‘Peculiar’ RRd stars observed by <i>K2</i> Open
Four stars pulsating simultaneously with a dominant period PD ∈ (0.28, 0.39) d and an additional period PA ∈ (0.20, 0.27) d have been identified from among the more than 3000 RR Lyrae stars observed by the Kepler space telescope during NAS…
View article: Rotation and pulsation in Ap stars: first light results from TESS sectors 1 and 2
Rotation and pulsation in Ap stars: first light results from TESS sectors 1 and 2 Open
We present the first results from the Transiting Exoplanet Survey Satellite (TESS) on the rotational and pulsational variability of magnetic chemically peculiar A-type stars. We analyse TESS 2-min cadence data from sectors 1 and 2 on a sam…
View article: K2 Observations of Galactic RRd Stars
K2 Observations of Galactic RRd Stars Open
We have analysed high-precision photometry of 77 double-mode RR Lyrae (RRd) stars observed by NASA’s Kepler-K2 mission during Campaigns 1-18. Among those stars, we have identified several low-period ratio variables, belonging either to a s…
View article: K2 Observations of Double-Mode RR Lyrae Stars
K2 Observations of Double-Mode RR Lyrae Stars Open
View article: Little Bear's Pulsating Stars: Variable Star Census of dSph UMi Galaxy
Little Bear's Pulsating Stars: Variable Star Census of dSph UMi Galaxy Open
Recent observations and a photometric search for variable stars in the Ursa Minor dwarf spheroidal galaxy (UMi dSph) are presented. Our observations were taken at Apache Point Observatory in 2014 and 2016 using the 0.5m ARCSAT telescope an…
View article: Little Bear’s pulsating stars: Variable star census of UMi dSph Galaxy
Little Bear’s pulsating stars: Variable star census of UMi dSph Galaxy Open
\nRecent observations and a photometric search for variable stars in the Ursa Minor dwarf spheroidal galaxy (UMi dSph) are presented. Our observations were taken at Apache Point Observatory in 2014 and 2016 using the 0.5m ARCSAT telescope …
View article: Metal-rich SX Phe stars in the<i>Kepler</i>field
Metal-rich SX Phe stars in the<i>Kepler</i>field Open
A spectroscopic and photometric analysis has been carried out for thirty-two\ncandidate SX_Phe variable blue straggler stars in the Kepler-field (Balona &\nNemec 2012). Radial velocities (RVs), space motions (U,V,W), projected rotation\nve…
View article: The hot γ Doradus and Maia stars
The hot γ Doradus and Maia stars Open
The hot γ Doradus stars have multiple low frequencies characteristic of γ Dor or SPB variables, but are located between the red edge of the SPB and the blue edge of the γ Dor instability strips where all low-frequency modes are stable in c…
View article: An RR Lyrae family portrait: 33 stars observed in Pisces with K2-E2
An RR Lyrae family portrait: 33 stars observed in Pisces with K2-E2 Open
A detailed analysis is presented of 33 RR Lyrae stars in Pisces observed with the Kepler space telescope over the 8.9-d long K2 Two-Wheel Concept Engineering Test. The sample includes not only fundamental-mode and first-overtone (RRab and …
View article: Kepler photometry of RRc stars: peculiar double-mode pulsations and period doubling
Kepler photometry of RRc stars: peculiar double-mode pulsations and period doubling Open
We present the analysis of four first overtone RR Lyrae stars observed with the Kepler space telescope, based on data obtained over nearly 2.5 yr. All four stars are found to be multiperiodic. The strongest secondary mode with frequency f2…
View article: Metal-Rich SX Phe Stars in the<i>Kepler</i>Field
Metal-Rich SX Phe Stars in the<i>Kepler</i>Field Open
High-resolution spectroscopic observations have been made for 32 of the 34 candidate SX Phe stars identified in the Kepler field by Balona & Nemec (2012). All available long-and short-cadence Q0-Q17 Kepler photometry has been analyzed for …
View article: Ground-Based<i>BVRI</i>Time-Series Follow-Up Observations for the RR Lyrae stars in<i>Kepler</i>Field
Ground-Based<i>BVRI</i>Time-Series Follow-Up Observations for the RR Lyrae stars in<i>Kepler</i>Field Open
Time series observations for the 41 RR Lyrae stars in Kepler’s fields were carried out in 2010 to 2013 using a number of meter class (or smaller) telescopes. These telescopes include the 1-m and 41-cm telescopes of Lulin Observatory (LOT a…