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Symbiotic stars are interacting binary systems, making them valuable for studying various astronomical phenomena, such as stellar evolution, mass transfer, and accretion processes. Despite recent progress in the discovery of symbiotic…

太阳与恒星天体物理 · 物理学 2023-07-20 Yongle Jia , Sufen Guo , Chunhua Zhu , Lin Li , Mei Ma , Guoliang Lv

Symbiotic stars are interacting binary systems with the longest orbital periods. They are typically formed by a white dwarf, a red giant and a nebula. These objects are natural astrophysical laboratories for studying the evolution of…

Symbiotic star (SySt) is long-period interacting binary system, typically consisting of a white dwarf and a red giant surrounded by a nebula. These systems are natural astrophysical laboratories for investigating binary star evolution. In…

太阳与恒星天体物理 · 物理学 2025-06-12 Jing Chen , Liang Wang , Yin-Bi Li , Xiao-Xiao Ma , A-Li Luo , Zi-Chong Zhang , Ming-Yi Ding , Kai Zhang

Symbiotic stars belong to a group of interacting binaries that display a wide variety of phenomena, including prominent outbursts connected with mass transfer, as well as stellar winds, jets, eclipses, or intrinsic variability of the…

太阳与恒星天体物理 · 物理学 2021-08-11 J. Merc , R. Gális , M. Wolf , P. Velez , C. Buil , F. Sims , T. Bohlsen , M. Vrašťák , C. Boussin , H. Boussier , P. Cazzato , I. Diarrasouba , F. Teyssier

Yellow symbiotic stars are useful targets to probe whether mass transfer has happened in these binary systems. However, the number of known yellow symbiotic stars is very scarce. We report spectroscopic observations of five candidate yellow…

太阳与恒星天体物理 · 物理学 2016-04-13 N. O. Baella , C. B. Pereira , L. F. Miranda , A. Alvarez-Candal

Symbiotic stars (SySts) are interacting binaries composed of a red giant transferring material to a hot compact star, typically a white dwarf. Although only about 300 systems are confirmed, the Galactic population is estimated at 1.2 x 10^3…

We report the validation of a recently proposed infrared selection criterion for symbiotic stars (SySts). Spectroscopic data were obtained for seven candidates, selected from the SySt candidates of Akras et al. (2019, MNRAS, 483, 5077) by…

太阳与恒星天体物理 · 物理学 2021-02-17 Stavros Akras , Denise R. Gonçalves , Alvaro Alvarez-Candal , Claudio B. Pereira

We introduce the first results from an ongoing, systematic survey for new symbiotic stars selected from the AAO/UKST SuperCOSMOS H$\alpha$ Survey (SHS). The survey aims to identify and characterise the fainter population of symbiotic stars…

太阳与恒星天体物理 · 物理学 2015-06-17 Brent Miszalski , Joanna Mikołajewska

We present the continuation of a systematic search for new southern Galactic symbiotic stars, selecting candidates from the SuperCOSMOS H$\alpha$ Survey and 2MASS. Follow-up spectroscopy with the Southern African Large Telescope (SALT) was…

太阳与恒星天体物理 · 物理学 2025-12-19 J. Merc , J. Mikołajewska , K. Iłkiewicz , B. Monard , A. Udalski

The study of symbiotic stars is essential to understand important aspects of stellar evolution in interacting binaries. Their observed population in the Galaxy is however poorly known, and is one to three orders of magnitudes smaller than…

Symbiotic stars, interacting binaries composed of a cool giant and a hot compact companion, exhibit complex variability across the electromagnetic spectrum. Over the past decades, large-scale photometric and spectroscopic surveys from…

太阳与恒星天体物理 · 物理学 2025-04-24 Jaroslav Merc

Symbiotic stars, binary pairs with a cool giant fueling accretion onto a hot compact companion, offer unique insights to our understanding of stellar evolution. Yet, only a few hundred symbiotic stars are confirmed. Here, we report on a new…

太阳与恒星天体物理 · 物理学 2025-08-27 Samantha E. Ball , Benjamin C. Bromley , Scott J. Kenyon

In a previous paper [arXiv:0712.2391], we presented the selection criteria needed to search for symbiotic stars in IPHAS, the INT Halpha survey of the Northern Galactic plane. IPHAS gives us the opportunity to make a systematic, complete…

Just less than 300 symbiotic stars are currently known in the Galaxy. The population synthesis methods predict that this amount should be 10--100 times larger. In recent years, several works have attempted to find symbiotic candidates from…

太阳与恒星天体物理 · 物理学 2025-03-18 A. M. Tatarnikov , A. A. Tatarnikova , N. A. Maslennikova , A. V. Dodin , M. A. Burlak , A. A. Tatarnikov

Symbiotic stars (SySts) are long-period interacting binaries composed of a hot compact star, an evolved giant star, and a tangled network of gas and dust nebulae. They represent unique laboratories for studying a variety of important…

We are performing a search for symbiotic stars using IPHAS, the INT Halpha survey of the northern Galactic plane, and follow-up observations. Candidate symbiotic stars are selected on the basis of their IPHAS and near-IR colours, and…

太阳与恒星天体物理 · 物理学 2011-04-08 R. L. M. Corradi , L. Sabin , U. Munari , G. Cetrulo , A. Englaro , R. Angeloni , R. Greimel , A. Mampaso

Theoretical predictions of the population of Galactic symbiotic stars (SySts) are highly inconsistent with the current known population. Despite intense effort over the past decades, observations are still far below the predictions. The…

太阳与恒星天体物理 · 物理学 2023-01-20 Stavros Akras

Symbiotic binaries are putative progenitors of type Ia supernovae. The census of Galactic symbiotic binaries is so incomplete that we cannot reliably estimate the total population of these stars, and use it to check whether that number is…

太阳与恒星天体物理 · 物理学 2015-06-19 Joanna Mikolajewska , Nelson Caldwell , Michael M. Shara

Symbiotic stars are interacting binaries with the longest orbital periods and their multi-component structure makes them rich astrophysical laboratories. The accretion of a high mass loss rate red giant wind on to a white dwarf (WD) makes…

太阳与恒星天体物理 · 物理学 2013-05-22 Brent Miszalski , Joanna Mikołajewska , Andrzej Udalski

We present a new catalogue of symbiotic stars. In our list we include 188 symbiotic stars as well as 28 objects suspected of being symbiotic. For each star, we present basic observational material: coordinates, V and K magnitudes,…

天体物理学 · 物理学 2009-10-31 K. Belczynski , J. Mikolajewska , U. Munari , R. J. Ivison , M. Friedjung
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