scholarly journals Combining BRITE and ground-based photometry for the β Cephei star ν Eridani: impact on photometric pulsation mode identification and detection of several g modes

2016 ◽  
Vol 464 (2) ◽  
pp. 2249-2258 ◽  
Author(s):  
G. Handler ◽  
M. Rybicka ◽  
A. Popowicz ◽  
A. Pigulski ◽  
R. Kuschnig ◽  
...  
Keyword(s):  
Mode Identification ◽  
Pulsation Mode

scholarly journals The fast rotating δ Scuti pulsator V376 Per: Frequency analysis and mode identification

2013 ◽  
Vol 9 (S301) ◽  
pp. 499-500
Author(s):  
Nathalie Themessl ◽  
Veronique Fritz ◽  
Michel Breger ◽  
Sabine Karrer ◽  
Barbara G. Castanheira
Keyword(s):  
High Resolution ◽  
Line Profile ◽  
Frequency Analysis ◽  
Spectroscopic Data ◽  
Simultaneous Analysis ◽  
Stellar Spectra ◽  
Mode Identification ◽  
Pulsation Mode ◽  
Scuti Star ◽  
Fast Rotating

AbstractOur simultaneous analysis of ground-based photometric and high-resolution spectroscopic data of the δ Scuti star V376 Per revealed eight individual frequencies from 82 nights of two-color photometry and six frequencies from the line-profile variations using 769 stellar spectra. Additionally, we identified the corresponding pulsation modes and derived reliable estimates of the line profile and pulsation mode parameters.

scholarly journals Identification of pulsation modes from spectroscopy

2013 ◽  
Vol 9 (S301) ◽  
pp. 101-107 ◽  
Author(s):  
Katrien Uytterhoeven
Keyword(s):  
Time Series ◽  
High Resolution ◽  
Data Quality ◽  
Spectroscopic Data ◽  
Main Sequence ◽  
Mode I ◽  
Mode Identification ◽  
Pulsation Mode ◽  
Identification Techniques

AbstractTime-series of high-resolution spectra of massive main-sequence pulsators contain information on the degree l and azimuthal number m of a pulsation mode. I present an overview of existing mode-identification techniques that have been developed to derive l and m from spectroscopic data. I also discuss the data quality needed to perform such a study. Through some examples from the literature I show that the optimal way to identify modes in heat-driven non-radial pulsators is by 1) using multi-site campaign data, 2) combining different spectroscopic mode-identification techniques, and 3) combining results from photometric and spectroscopic mode-identification studies.

On the Pulsation Mode Identification of Short-Period Galactic Cepheids

2001 ◽  
Vol 552 (2) ◽  
pp. L141-L145 ◽  
Author(s):  
G. Bono ◽  
W. P. Gieren ◽  
M. Marconi ◽  
P. Fouqué
Keyword(s):  
Mode Identification ◽  
Pulsation Mode ◽  
Short Period

scholarly journals Mode Identification in the δ Scuti Star 20 CVn

2002 ◽  
Vol 185 ◽  
pp. 334-335
Author(s):  
M. Chadid ◽  
P. Mathias ◽  
J. De Ridder ◽  
C. Aerts
Keyword(s):  
Spectroscopic Study ◽  
Mode Identification ◽  
Pulsation Mode ◽  
Scuti Star

AbstractWe present a new Spectroscopic study of the δ Scuti star 20 CVn in order to solve the controversy on the type of pulsation mode of this object.

scholarly journals Mode Identification of the β Cephei star BW Vulpeculae

1995 ◽  
Vol 155 ◽  
pp. 56-57
Author(s):  
C. Aerts ◽  
T. Van Hoolst ◽  
P. Mathias
Keyword(s):  
Moment Method ◽  
Radial Pulsation ◽  
Mode Identification ◽  
Pulsation Mode ◽  
Non Linear ◽  
Linear Behaviour ◽  
The Moment

AbstractWe identify the pulsation mode of BW Vul by means of both the moment method and the method of photometric amplitudes and find a radial pulsation. We briefly study the non-linear behaviour of BW Vul.

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