Abundance analysis and searching for nonradial pulsations in the atmosphere of the chemically peculiar star HD 115708

2008 ◽  
Vol 34 (6) ◽  
pp. 413-422 ◽  
Author(s):  
E. A. Semenko ◽  
M. E. Sachkov ◽  
T. A. Ryabchikova ◽  
D. O. Kudryavtsev ◽  
N. E. Piskunov
Keyword(s):  
Peculiar Star ◽  
Chemically Peculiar

Very High Resolution Ultraviolet Spectroscopy of a Chemically Peculiar Star: Results of the χ Lupi Pathfinder Project

1999 ◽  
Vol 117 (3) ◽  
pp. 1454-1470 ◽  
Author(s):  
David S. Leckrone ◽  
Charles R. Proffitt ◽  
Glenn M. Wahlgren ◽  
Sveneric G. Johansson ◽  
Tomas Brage
Keyword(s):  
High Resolution ◽  
Ultraviolet Spectroscopy ◽  
Peculiar Star ◽  
Chemically Peculiar ◽  
Very High

scholarly journals An update on the rotational period of the magnetic chemically peculiar star CU Virginis

2013 ◽  
Vol 431 (3) ◽  
pp. 2106-2110 ◽  
Author(s):  
Diane M. Pyper ◽  
Ian R. Stevens ◽  
Saul J. Adelman
Keyword(s):  
Rotational Period ◽  
Peculiar Star ◽  
Chemically Peculiar

scholarly journals A search for rapid pulsations in the magnetic cool chemically peculiar star HD 3980★

2008 ◽  
Vol 390 (3) ◽  
pp. 1250-1257 ◽  
Author(s):  
V. G. Elkin ◽  
D. W. Kurtz ◽  
L. M. Freyhammer ◽  
S. Hubrig ◽  
G. Mathys
Keyword(s):  
Peculiar Star ◽  
Chemically Peculiar

scholarly journals Study of Inhomogeneities on the Surface of Magnetic CP Stars

1986 ◽  
Vol 90 ◽  
pp. 125-132
Author(s):  
V.L. Khokhlova
Keyword(s):  
Magnetic Field ◽  
Inverse Problem ◽  
Stokes Parameters ◽  
Abundance Distribution ◽  
Peculiar Star ◽  
Chemically Peculiar ◽  
Field Geometry

AbstractThe formulation and solution of the inverse problem to determine local Stokes parameters on the surface of a star, in particular magnetic chemically peculiar star, and hence to determine surface abundance distribution and magnetic field geometry is reviewed.

The Advanced Spectral Library (ASTRAL): Abundance Analysis of the Chemically Peculiar Star HR 465

2020 ◽  
Vol 899 (2) ◽  
pp. 166
Author(s):  
Krister E. Nielsen ◽  
Kenneth G. Carpenter ◽  
Gladys V. Kober ◽  
Glenn M. Wahlgren
Keyword(s):  
Spectral Library ◽  
Peculiar Star ◽  
Chemically Peculiar

scholarly journals A spectroscopic analysis of the chemically peculiar star HD 207561

2012 ◽  
Vol 424 (3) ◽  
pp. 2002-2008 ◽  
Author(s):  
S. Joshi ◽  
E. Semenko ◽  
P. Martinez ◽  
M. Sachkov ◽  
Y. C. Joshi ◽  
...  
Keyword(s):  
Spectroscopic Analysis ◽  
Peculiar Star ◽  
Chemically Peculiar

scholarly journals Critical Complements: Progress on the Orbit of T Mon

2000 ◽  
Vol 176 ◽  
pp. 246-247
Author(s):  
N. R. Evans ◽  
K. Carpenter ◽  
R. Robinson ◽  
D. Massa ◽  
G. M. Wahlgren ◽  
...  
Keyword(s):  
Orbital Motion ◽  
High Luminosity ◽  
Peculiar Star ◽  
Classical Cepheid ◽  
Chemically Peculiar ◽  
Short Period

AbstractA preliminary orbit has been derived for the high luminosity, 27-d classical Cepheid T Mon. Velocities for the hot companion have been measured from an HST GHRS spectrum and 3 IUE spectra. The companion velocities are inconsistent with binary orbital motion and it is likely that the companion is itself a short period binary. The HST spectrum also shows that the companion is a chemically peculiar star, probably magnetic.

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