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相关论文: Gaia18aen: First symbiotic star discovered by Gaia

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In this work, we present the discovery and characterization of a new southern S-type symbiotic star, DeGaPe 35. We have obtained the low-resolution spectroscopic observations and supplemented them with photometry from Gaia DR3 and other…

We report the discovery of the optical dipper and low-luminosity infrared stellar transient Gaia20ehk (hereafter, Gaia-GIC-1), which is currently undergoing high-amplitude variability due to transiting dusty material. In this work, we…

地球与行星天体物理 · 物理学 2026-03-12 Anastasios Tzanidakis , James R. A. Davenport

The Gaia Alert System issued an alert on 2020 August 28, on Gaia 20eae when its light curve showed a $\sim$4.25 magnitude outburst. We present multi-wavelength photometric and spectroscopic follow-up observations of this source since 2020…

The spectral and photometric studies of the cataclysmic variable Gaia 19cwm (or ZTF19aamkwxk) have been performed. Based on the analysis of long-term variability, it is concluded that the object belongs to WZ Sge type stars. The light…

Since July 2014, the Gaia mission has been engaged in a high-spatial-resolution, time-resolved, precise, accurate astrometric, and photometric survey of the entire sky. Aims: We present the Gaia Science Alerts project, which has been in…

天体物理仪器与方法 · 物理学 2021-08-18 S. T. Hodgkin , D. L. Harrison , E. Breedt , T. Wevers , G. Rixon , A. Delgado , A. Yoldas , Z. Kostrzewa-Rutkowska , Ł. Wyrzykowski , M. van Leeuwen , N. Blagorodnova , H. Campbell , D. Eappachen , M. Fraser , N. Ihanec , S. E. Koposov , K. Kruszyńska , G. Marton , K. A. Rybicki , A. G. A. Brown , P. W. Burgess , G. Busso , S. Cowell , F. De Angeli , C. Diener , D. W. Evans , G. Gilmore , G. Holland , P. G. Jonker , F. van Leeuwen , F. Mignard , P. J. Osborne , J. Portell , T. Prusti , P. J. Richards , M. Riello , G. M. Seabroke , N. A. Walton , Péter Ábrahám , G. Altavilla , S. G. Baker , U. Bastian , P. O'Brien , J. de Bruijne , T. Butterley , J. M. Carrasco , J. Castañeda , J. S. Clark , G. Clementini , C. M. Copperwheat , M. Cropper , G. Damljanovic , M. Davidson , C. J. Davis , M. Dennefeld , V. S. Dhillon , C. Dolding , M. Dominik , P. Esquej , L. Eyer , C. Fabricius , M. Fridman , D. Froebrich , N. Garralda , A. Gomboc , J. J. González-Vidal , R. Guerra , N. C. Hambly , L. K. Hardy , B. Holl , A. Hourihane , J. Japelj , D. A. Kann , C. Kiss , C. Knigge , U. Kolb , S. Komossa , Á. Kóspál , G. Kovács , M. Kun , G. Leto , F. Lewis , S. P. Littlefair , A. A. Mahabal , C. G. Mundell , Z. Nagy , D. Padeletti , L. Palaversa , A. Pigulski , M. L. Pretorius , W. van Reeven , V. A. R. M. Ribeiro , M. Roelens , N. Rowell , N. Schartel , A. Scholz , A. Schwope , B. M. Sipőcz , S. J. Smartt , M. D. Smith , I. Serraller , D. Steeghs , M. Sullivan , L. Szabados , E. Szegedi-Elek , P. Tisserand , L. Tomasella , S. van Velzen , P. A Whitelock , R. W. Wilson , D. R. Young

We report the serendipitous discovery of Gaia17bpp/2MASS J19372316+1759029, a star with a deep single large-amplitude dimming event of $\sim$4.5 magnitudes that lasted over 6.5 years. Using the optical to IR spectral energy distribution…

太阳与恒星天体物理 · 物理学 2023-06-22 Anastasios Tzanidakis , James R. A. Davenport , Eric C. Bellm , Yuankun Wang

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

V2756 Sgr is a long-known S-type symbiotic binary that was recently detected in $\sim$ 1 mag eclipse-like fading by the Gaia satellite. This behavior was reported as a Gaia Science Alert under the designation Gaia22eor. V2756 Sgr has not…

太阳与恒星天体物理 · 物理学 2022-12-09 Jaroslav Merc , Hamish Barker , Rudolf Gális

Context. Among known young stellar objects (YSOs), those exhibiting the most dramatic increases in brightness due to sudden increase in mass accretion rate are eruptive young stars. Gaia20dsk is one of the Gaia-alerted young star candidates…

Young stars show variability on different time-scales from hours to decades, with a range of amplitudes. We studied two young stars, which triggered the Gaia Science Alerts system due to brightenings on a time-scale of a year. Gaia20bwa…

We report on the source Gaia 19ajj, identifying it as a young star associated with a little-studied star-forming region seen along a complex line-of-sight through the Gum Nebula. The optical lightcurve recently recorded by Gaia exhibits a…

太阳与恒星天体物理 · 物理学 2020-01-08 Lynne A. Hillenbrand , Bo Reipurth , Michael Connelley , Roc M. Cutri , Howard Isaacson

Gaia is the cornerstone mission of the European Space Agency. From late 2013 it will start collecting superb astrometric, photometric and spectroscopic data for around a billion of stars of our Galaxy. While surveying the whole sky down to…

天体物理仪器与方法 · 物理学 2012-10-23 Lukasz Wyrzykowski , Simon Hodgkin , Nadejda Blogorodnova , Sergey Koposov , Ross Burgon

The poorly studied variable star V390 Sco, previously classified as a Mira pulsator, was detected in a brightening event by the ESA Gaia satellite in September 2023. This work presents an analysis of available archival multifrequency…

太阳与恒星天体物理 · 物理学 2024-03-22 Jaroslav Merc , Peter Velez , Stéphane Charbonnel , Olivier Garde , Pascal Le Dû , Lionel Mulato , Thomas Petit , Jan Skowron

The ESA Gaia satellite scans the whole sky with a temporal sampling ranging from seconds and hours to months. Each time a source passes within the Gaia field of view, it moves over 10 CCDs in 45 s and a lightcurve with 4.5 s sampling (the…

We present the results of the optical study of the new eclipsing polar Gaia23cer. We analyzed the brightness variability of the polar in high ($\langle r \rangle \approx 16.5\mathrm{\,mag}$) and low ($\langle r \rangle \approx…

We present ultraviolet, optical and infrared photometry and optical spectroscopy of the type Ic superluminous supernova (SLSN) Gaia16apd (= SN 2016eay), covering its evolution from 26 d before the $g$-band peak to 234.1 d after the peak.…

Supernova (SN) 2018oh (ASASSN-18bt) is the first spectroscopically-confirmed type Ia supernova (SN Ia) observed in the $Kepler$ field. The $Kepler$ data revealed an excess emission in its early light curve, allowing to place interesting…

太阳与恒星天体物理 · 物理学 2019-01-09 W. Li , X. Wang , J. Vinkó , J. Mo , G. Hosseinzadeh , D. J. Sand , J. Zhang , H. Lin , T. Zhang , L. Wang , J. Zhang , Z. Chen , D. Xiang , L. Rui , F. Huang , X. Li , X. Zhang , L. Li , E. Baron , J. M. Derkacy , X. Zhao , H. Sai , K. Zhang , L. Wang , D. A. Howell , C. McCully , I. Arcavi , S. Valenti , D. Hiramatsu , J. Burke , A. Rest , P. Garnavich , B. E. Tucker , G. Narayan , E. Shaya , S. Margheim , A. Zenteno , A. Villar , G. Dimitriadis , R. J. Foley , Y. -C. Pan , D. A. Coulter , O. D. Fox , S. W. Jha , D. O. Jones , D. N. Kasen , C. D. Kilpatrick , A. L. Piro , A. G. Riess , C. Rojas-Bravo , B. J. Shappee , T. W. -S. Holoien , K. Z. Stanek , M. R. Drout , K. Auchettl , C. S. Kochanek , J. S. Brown , S. Bose , D. Bersier , J. Brimacombe , P. Chen , S. Dong , S. Holmbo , J. A. Muñoz , R. L. Mutel , R. S. Post , J. L. Prieto , J. Shields , D. Tallon , T. A. Thompson , P. J. Vallely , S. Villanueva , S. J. Smartt , K. W. Smith , K. C. Chambers , H. A. Flewelling , M. E. Huber , E. A. Magnier , C. Z. Waters , A. S. B. Schultz , J. Bulger , T. B. Lowe , M. Willman , K. Sárneczky , A. Pál , J. C. Wheeler , A. Bódi , Zs. Bognár , B. Csák , B. Cseh , G. Csörnyei , O. Hanyecz , B. Ignácz , Cs. Kalup , R. Könyves-Tóth , L. Kriskovics , A. Ordasi , I. Rajmon , A. Sódor , R. Szabó , R. Szakáts , G. Zsidi , P. Milne , J. E. Andrews , N. Smith , C. Bilinski , P. J. Brown , J. Nordin , S. C. Williams , L. Galbany , J. Palmerio , I. M. Hook , C. Inserra , K. Maguire , Régis Cartier , A. Razza , C. P. Gutiérrez , J. J. Hermes , J. S. Reding , B. C. Kaiser , J. L. Tonry , A. N. Heinze , L. Denneau , H. Weiland , B. Stalder , G. Barentsen , J. Dotson , T. Barclay , M. Gully-Santiago , C. Hedges , A. M. Cody , S. Howell , J. Coughlin , J. E. Van Cleve , J. Vinícius de Miranda Cardoso , K. A. Larson , K. M. McCalmont-Everton , C. A. Peterson , S. E. Ross , L. H. Reedy , D. Osborne , C. McGinn , L. Kohnert , L. Migliorini , A. Wheaton , B. Spencer , C. Labonde , G. Castillo , G. Beerman , K. Steward , M. Hanley , R. Larsen , R. Gangopadhyay , R. Kloetzel , T. Weschler , V. Nystrom , J. Moffatt , M. Redick , K. Griest , M. Packard , M. Muszynski , J. Kampmeier , R. Bjella , S. Flynn , B. Elsaesser

Context. Gaia18cjb is one of the Gaia-alerted eruptive young star candidates which has been experiencing a slow and strong brightening during the last 13 years, similar to some FU Orionis-type objects. Aims. The aim of this work is to…

We present photometric follow-up observations of the supernova candidate AT 2018we, which was discovered by the Gaia photometric alerts system. The first Gaia detection of the object was made Feb 12, 2018. Our observations, made in Cousins…

太阳与恒星天体物理 · 物理学 2018-09-18 T. Willamo , J. Ala-Könni , J. Arvo , I. Pippa , T. Salo
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