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Chemically peculiar star
Orbit of the Mercury-Manganese Binary 41 Eridani? C
N O T I C E This Document Has Been Reproduced From
Chandra X-Ray Study Confirms That the Magnetic Standard Ap Star KQ Vel
10252228.Pdf
KELT-17: a Chemically Peculiar Am Star and a Hot-Jupiter Planet
Constraining the Very Heavy Elemental Abundance Peak in the Chemically Peculiar Star Lupi, with New Atomic Data for Os II and Ir II
Rotational Modulation of Light Star Spots - Ii Star Spots 2
Chemically Peculiar Star HR8844 Could Be a Hybrid Object 21 September 2016, by Tomasz Nowakowski
HD 158450: the Magnetic Chemically Peculiar Star in a Young Stellar Group
Arxiv:2006.03329V1 [Astro-Ph.SR] 5 Jun 2020 1
Mass Transfer in Binary Stars
A Frequency Analysis of the Rapidly Oscillating Ap Star HD 101065
Ankara Üniversitesi Fen Bilimleri Enstitüsü Yüksek
Physical Properties of a Complete Volume-Limited
STARS2016: Understanding the Roles of Rotation, Pulsation and Chemical Peculiarities in the Upper Main Sequence
THE OBSERVATORY Founded in by Sir William Christie, Astronomer Royal
Measuring Stellar Magnetic Fields from High Resolution Spectroscopy Of
Chemically Peculiar Stars in the Large Magellanic Cloud⋆
Top View
Understanding the Rotational Variability of K2 Targets
A Magnetic Bp Star in an Eclipsing Binary with a Non-Magnetic ‘Identical Twin’
The Most Metal-Poor Stars. II. Chemical Abundances of 190 Metal-Poor Stars Including 10 New Stars with [Fe/H] ≤ -3.5
Magnetic Fields Discovered in Two Hot Evolved Stars 3 January 2018, by Tomasz Nowakowski
The COLOUR of CREATION Observing and Astrophotography Targets “At a Glance” Guide
Indirect Imaging of Ultra-Cool Dwarfs
KELT-17: a Chemically Peculiar Am Star and a Hot-Jupiter Planet? C
Chemically Peculiar Stars: the Binary/CEMP Connection
Saul J. Adelman
The Nature of Light Variations in Magnetic Hot Stars J
Abundance Pattern of the Chemically Peculiar Star Feh-Duf
Readily Be Attributed to the Choice of Abundances Used in the Spectral fitting
Spectral Study of V565 Mon: Probable FU Ori-Like Or Chemically Peculiar Star
The Angular Diameter of Lambda Bootis
Étude Expérimentale Et Théorique Des Spectres D'émission VUV Des Ions
An Abundance Analysis of a Chemically Peculiar B Star – JL 87*,**
Λ Bootis Stars ISM Gas Accretion As an Explanation for Chemical Peculiarity
A Probable Pre-Main Sequence Chemically Peculiar Star in the Open Cluster Stock 16