强恒星和太阳耀斑中白光连续体发射源的研究

IF 0.7 4区物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS

Astrophysics Pub Date : 2026-04-23 DOI:10.1007/s10511-026-09906-4

E. S. Morchenko

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引用次数: 0

摘要

在本研究中，我们注意到在dMe恒星和太阳上的强耀斑期间存在两个不同时间发展的独立区域的一些可观测表现。我用经典的光曲线对强大的恒星耀斑中白光连续体的起源提出了一个理论解释，并结合对太阳上第一类白光耀斑的观测进行了讨论。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

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On the Origin of Emission in the White-Light Continuum in Powerful Stellar and Solar Flares

In this study, attention is drawn to some observable manifestations of the existence of two separate regions with different temporal development during powerful flares on dMe stars and on the Sun. I propose a theoretical interpretation of the origin of the white-light continuum in powerful stellar flares with classical light curves and discuss it in the context of observations of the white-light flares of the first type on the Sun.

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来源期刊

Astrophysics 地学天文-天文与天体物理

CiteScore

0.90

自引率

20.00%

发文量

审稿时长

6-12 weeks

期刊介绍： Astrophysics (Ap) is a peer-reviewed scientific journal which publishes research in theoretical and observational astrophysics. Founded by V.A.Ambartsumian in 1965 Astrophysics is one of the international astronomy journals. The journal covers space astrophysics, stellar and galactic evolution, solar physics, stellar and planetary atmospheres, interstellar matter. Additional subjects include chemical composition and internal structure of stars, quasars and pulsars, developments in modern cosmology and radiative transfer.