Pushing the limit of instrument capabilities
Denis V. Shulyak (1), Werner W. Weiss (2), Gautier Mathys (3), Laurent, Eyer (4), Alexander F. Kholtygin (5), Oleg Kochukhov (6), Pierre North (7),, Sergey N. Fabrika (8), Tatyana E. Burlakova (8) ((1)Institute of, Astrophysics, Georg-August-University, Germany
TL;DR
This paper reviews recent advances in Chemically Peculiar star research, highlighting ground-based observational successes and discussing future prospects with upcoming space missions like Gaia.
Contribution
It provides an overview of recent ground-based findings and explores the potential impact of the Gaia space mission on CP star studies.
Findings
Recent ground-based observations have advanced understanding of CP stars.
Pulsation phenomena have been identified in some cool CP stars.
Future Gaia mission will significantly enhance CP star research.
Abstract
Chemically Peculiar (CP) stars have been subject of systematic research since more than 50 years. With the discovery of pulsation of some of the cool CP stars, the availability of advanced spectropolarimetric instrumentation and high signal- to-noise, high resolution spectroscopy, a new era of CP star research emerged about 20 years ago. Together with the success in ground-based observations, new space projects are developed that will greatly benefit for future investigations of these unique objects. In this contribution we will give an overview of some interesting results obtained recently from ground-based observations and discuss on future outstanding Gaia space mission and its impact on CP star research.
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