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相关论文: Flickering of the jet-ejecting symbiotic star MWC …

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It is widely accepted that strong and variable radiation detected over all accessible energy bands in a number of active galaxies arises from a relativistic, Doppler-boosted jet pointing close to our line of sight. The size of the emitting…

宇宙学与河外天体物理 · 物理学 2010-11-19 LAT Collaboration , members of the 3C 279 multi-band campaign

Symbiotic binaries are long period interacting binaries consisting of a white dwarf (WD) accreting material from a cool evolved giant star via stellar winds. In this paper we study the symbiotic binary LIN 358 located in the SMC. We have…

太阳与恒星天体物理 · 物理学 2020-11-18 J. Kuuttila , M. Gilfanov , T. E. Woods , I. R. Seitenzahl , A. J. Ruiter

We present time-series VLT spectroscopy and NTT photometry of the cataclysmic variable SDSS J220553.98+115553.7, which contains a pulsating white dwarf. We determine a spectroscopic orbital period of 82.825 +/- 0.089 min from velocity…

天体物理学 · 物理学 2009-11-13 John Southworth , D W Townsley , B T Gaensicke

We conducted 4-night multiwavelength observations of an active M-dwarf star EV Lac on 2022 October 24$-$27 with simultaneous coverage of soft X-rays (NICER; 0.2$-$12 $\mathrm{keV}$, Swift XRT; 0.2$-$10 $\mathrm{keV}$), near-ultraviolet…

We present projected rotational velocity measurements of the red giant in the symbiotic star MWC 560 (V694 Mon), using the high-resolution spectroscopic observations with the FEROS spectrograph. We find that the projected rotational…

太阳与恒星天体物理 · 物理学 2015-05-14 R. K. Zamanov , A. Gomboc , K. A. Stoyanov , I. K. Stateva

We report on X-ray flares that were observed from the active galactic nucleus I Zwicky 1 (I Zw 1) in 2020 January by the NuSTAR and XMM-Newton observatories. The X-ray spectrum is well-described by a model comprised of the continuum…

高能天体物理现象 · 物理学 2022-04-06 D. R. Wilkins , L. C. Gallo , E. Costantini , W. N. Brandt , R. D. Blandford

In this paper we present a temporal and spectral analysis of X-ray data from the XMM and Chandra observations of the ultrasoft and variable Seyfert galaxy RX J1301.9+2747. In both observations the source clearly displays two distinct states…

星系天体物理 · 物理学 2015-06-15 Luming Sun , Xinwen Shu , Tinggui Wang

The variation mechanism of blazars is a long standing open question. The polarization observation can provide us with more information to constrain models. In this work, we collect the long term multi-wavelength data of AO 0235+164, and…

高能天体物理现象 · 物理学 2020-10-21 Yifan Wang , Yunguo Jiang

We present surface photometry of a giant, low surface brightness stellar arc in the halo of the nearby spiral galaxy M63 (NGC 5055) that is consistent with being a part of a stellar stream resulting from the disruption of a dwarf satellite…

We present follow-up photometry and spectroscopy of ZTF J0328$-$1219 strengthening its status as a white dwarf exhibiting transiting planetary debris. Using TESS and Zwicky Transient Facility photometry, along with follow-up high speed…

(abridged) The heating mechanism at high densities during M dwarf flares is poorly understood. Spectra of M dwarf flares in the optical and near-ultraviolet wavelength regimes have revealed three continuum components during the impulsive…

太阳与恒星天体物理 · 物理学 2015-06-23 Adam F. Kowalski , Suzanne L. Hawley , Mats Carlsson , Joel C. Allred , Han Uitenbroek , Rachel A. Osten , Gordon Holman

Solar white-light flares (WLFs) are those accompanied by brightenings in the optical continuum or integrated light. The White-light Solar Telescope (WST), as an instrument of the Lyman-alpha Solar Telescope (LST) on the Advanced Space-based…

We report the serendipitous detection of a giant X-ray flare from the source 2XMM J043527.2-144301 during an XMM-Newton observation of the high latitude molecular cloud MBM20. The source has not been previously studied at any wavelength.…

太阳与恒星天体物理 · 物理学 2015-05-27 Anjali Gupta , Massimiliano Galeazzi , Benjamin Williams

We report results of the eclipse mapping analysis of an ensemble of light curves of HT Cas. The fast response of the white dwarf to the increase in mass transfer rate, the expansion rate of the accretion disc at the same time, and the…

太阳与恒星天体物理 · 物理学 2011-05-10 R. Baptista , B. Borges , V. Kolokotronis , O. Giannakis , C. J. Papadimitriou

We derive simple analytic expressions for the continuum lightcurves and spectra of flaring and flickering events that occur over a wide range of astrophysical systems. We compare these results to data taken from the cataclysmic variable SS…

天体物理学 · 物理学 2009-11-10 K. J. Pearson , Keith Horne , Warren Skidmore

AIMS: We investigated the optical variability of the symbiotic binary FN Sgr, with photometric monitoring during $\simeq$55 years and with a high-cadence Kepler light curve lasting 81 days. METHODS: The data obtained in the V and I bands…

太阳与恒星天体物理 · 物理学 2023-07-12 J. Magdolen , A. Dobrotka , M. Orio , J. Mikołajewska , A. Vanderburg , B. Monard , R. Aloisi , P. Bezák

We determine the phase diagram for dense carbon/ oxygen mixtures in White Dwarf (WD) star interiors using molecular dynamics simulations involving liquid and solid phases. Our phase diagram agrees well with predictions from Ogata et al. and…

太阳与恒星天体物理 · 物理学 2014-11-21 C. J. Horowitz , A. S. Schneider , D. K. Berry

We report on a large X-ray flare from the Lindroos binary system HD 560 during a pointed ROSAT PSPC observation. Strong magnetic activity is expected for the late-type component (a G dwarf star and post-T Tauri Star candidate). The system…

天体物理学 · 物理学 2007-05-23 B. Stelzer , N. Huelamo

We examine the emergent fluxes from helium-core white dwarfs following their evolution from the end of pre-white dwarf stages down to advanced cooling stages. For this purpose, we include a detailed treatment of the physics of the…

天体物理学 · 物理学 2009-11-07 R. D. Rohrmann , A. M. Serenelli , L. G. Althaus , O. G. Benvenuto

We present time-resolved optical and ultraviolet spectroscopy and photometry of V1460~Her, an eclipsing cataclysmic variable with a 4.99\,h orbital period and an overluminous K5-type donor star. The optical spectra show emission lines from…

太阳与恒星天体物理 · 物理学 2020-10-14 R. P. Ashley , T. R. Marsh , E. Breedt , B. T. Gaensicke , A. F. Pala , O. Toloza , P. Chote , John R. Thorstensen , M. R. Burleigh