New online database of symbiotic variables: Symbiotics in X-rays

被引：21

作者：

Merc, J. ^{[1
]}

Galis, R. ^{[1
]}

Wolf, M. ^{[2
]}

机构：

[1] Safarik Univ, Inst Phys, Fac Sci, Pk Angelinum 9, Kosice 04001, Slovakia

[2] Charles Univ Prague, Fac Math & Phys, Astron Inst, Prague, Czech Republic

来源：

ASTRONOMISCHE NACHRICHTEN | 2019年 / 340卷 / 07期

关键词：

binaries; symbiotic; catalogues; X-rays; NOVA V745 SCO; 1ST DETECTION; STARS; EMISSION; DISCOVERY; IDENTIFICATION;

D O I：

10.1002/asna.201913662

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Symbiotic variable stars belong to an interesting class of interacting binary systems. Since the beginning of this century, the systematic search for these objects has begun, and such surveys have led to discoveries of many new objects and dozens of candidates in the Milky Way and the Local Group. As the latest catalogue of symbiotic binaries is almost two decades old, we decided to prepare a new, online database of the galactic and extragalactic symbiotic systems. These objects are also known for their X-ray emission. For the purpose of this work, we have prepared a census of symbiotic binaries and their properties based on observations obtained by X-ray satellites in the previous decades. As our review has shown, the X-ray emission seems to be a common feature of symbiotic systems, preferentially detected from nearby sources.

引用

页码：598 / 606

页数：9

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