论文标题
基本天体物理学的无声革命
A Silent Revolution in Fundamental Astrophysics
论文作者
论文摘要
隆期校正零点的任意性是一个近一年历史的范式，导致了两个范式。 “降压校正必须始终为负”，“恒星的辐射幅度应该比其$ V $幅度更明亮”。两者都被认为是在IAU 2015年大会决议B2之前被认为有效的，该决议B2是一份革命文件，它取代了上述三个范式。本文的目的是启动对基本天体物理学的新见解和新的理解，并提出新的能力，以获得标准，更准确的恒星发光性，并从盖亚之后的时代的准确观察中获得更多的收益。获得的准确性将有助于推进恒星结构和进化论，以及银河系和乳腺外的研究，观察性宇宙学以及暗物质以及暗能量搜索。
Arbitrariness in the zero point of bolometric corrections is a nearly century-old paradigm leading to two more paradigms. "Bolometric corrections must always be negative," and "bolometric magnitude of a star ought to be brighter than its $V$ magnitude". Both were considered valid before IAU 2015 General Assembly Resolution B2, a revolutionary document that supersedes all three aforementioned paradigms. The purpose of this article is to initiate a new insight and a new understanding of the fundamental astrophysics and present new capabilities to obtain standard and more accurate stellar luminosities and gain more from accurate observations in the era after Gaia. The accuracy gained will aid in advancing stellar structure and evolution theories, and also Galactic and extragalactic research, observational cosmology and dark matter and dark energy searches.
