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We report the discovery of a highly X-ray variable AGN, RX J2217.9-5941. This object was bright during the ROSAT All-Sky Survey (RASS), during which a decrease in the count rate by a factor of 12 was observed. It was found to be much…

天体物理学 · 物理学 2009-11-06 D. Grupe , H. -C. Thomas , K. M. Leighly

We report time-series photometry for 16 variable stars located in the central part of the globular cluster NGC 6752. The sample includes 13 newly identified objects. The precision of our differential photometry ranges from 1 mmag at V=14.0…

太阳与恒星天体物理 · 物理学 2014-11-20 Janusz Kaluzny , Ian B. Thompson

A previously faint young stellar object (YSO), V557 Mon, rapidly brightened in late 2024 and is currently at least $\Delta G=3.3$ magnitudes brighter than its typical pre-outburst brightness. The ongoing outburst is identified in the Gaia…

太阳与恒星天体物理 · 物理学 2025-02-14 Adolfo S. Carvalho , Lynne A. Hillenbrand

We present the serendipitous discovery of a low luminosity nova occurring in a symbiotic binary star system in the Milky Way. We lay out the extensive archival data alongside new follow-up observations related to the stellar object V$^*$ CN…

太阳与恒星天体物理 · 物理学 2020-09-02 Lachlan Lancaster , Jenny Greene , Yuan-Sen Ting , Sergey E. Koposov , Benjamin J. S. Pope , Rachael L. Beaton

Context. This observational paper has been prepared in the context of the large multi-wavelength effort by many observers with the aim of following up the transient flaring event of V404 Cygni that took place for several weeks in 2015 June.…

高能天体物理现象 · 物理学 2016-02-03 Josep Martí , Pedro L. Luque-Escamilla , María T. García-Hernández

V1184 Tau (CB 34V) lies in the field of the Bok globule CB 34 and was discovered as a large amplitude variable in 1993. According to the first hypothesis of the variability of the star, it is a FU Orionis candidate erupted between 1951 and…

太阳与恒星天体物理 · 物理学 2015-10-21 E. H. Semkov , S. P. Peneva , S. I. Ibryamov

We report the detection of rapid wavelength and intensity variations of narrow components in absorption line profiles of the hot galactic supergiant P Cygni. During most of the time, in one week of observations, there were two such…

天体物理学 · 物理学 2009-11-07 Cornelis de Jager , Garik Israelian

We have conducted a 1.5 year-long variability study of the stars in the Cygnus OB2 association, the region in the northern hemisphere with the highest density of optically visible massive stars. The survey was conducted using four pointings…

太阳与恒星天体物理 · 物理学 2014-10-27 J. Salas , J. Maíz Apellániz , R. H. Barbá

We present results of high-cadence monitoring of the optical light curve of the nearby, Type Ia SN 2014J in M82 using the 2.3m Aristarchos telescope. $B$ and $V$-band photometry on days 15-18 after $t_{max}(B)$, obtained with a cadence of 2…

太阳与恒星天体物理 · 物理学 2015-12-09 A. Z. Bonanos , P. Boumis

We analyse a light curve of the symbiotic star BF Cyg, covering 114 years of its photometric history. The star had a major outburst around the year 1894. Since then the mean optical brightness of the system is in steady decline, reaching…

天体物理学 · 物理学 2009-11-13 Elia Leibowitz , Liliana Formiggini

Accretion in young stellar objects (YSOs) is at least partially episodic, i.e. periods with high accretion rates ('bursts') are interspersed by quiescent phases. These bursts manifest themselves as eruptive variability. Here we present a…

太阳与恒星天体物理 · 物理学 2015-06-12 Aleks Scholz , Dirk Froebrich , Kenneth Wood

We present the results of high-resolution optical spectroscopy, low-resolution near-IR spectroscopy and near-infrared speckle interferometry of the massive young stellar object candidate V645 Cyg, acquired to refine its fundamental…

We present the results of new X-ray observations of XMMU 122939.7+075333, the black hole (BH) in the globular cluster RZ 2109 in the Virgo Cluster galaxy NGC 4472. A combination of non-detections and marginal detections in several recent…

高能天体物理现象 · 物理学 2015-05-19 Thomas J. Maccarone , Arunav Kundu , Stephen E. Zepf , Katherine L. Rhode

We have obtained phase-resolved optical spectroscopy of the old nova, and asynchronous polar V1500 Cyg. These new data reveal discrete cyclotron humps from two different strength magnetic fields. One region has B = 72 MG, while the other…

太阳与恒星天体物理 · 物理学 2018-01-24 Thomas E. Harrison , Ryan K. Campbell

We present ~800 days of photometric monitoring of Boyajian's Star (KIC 8462852) from the All-Sky Automated Survey for Supernovae (ASAS-SN) and ~4000 days of monitoring from the All Sky Automated Survey (ASAS). We show that from 2015 to the…

We report on the short and long term X-ray properties of the bright nearby Seyfert 2 galaxy NGC 2992, which was extensively observed with Swift, XMM-Newton and NuSTAR. Swift targeted the source more than 100 times between 2019 and 2021 in…

高能天体物理现象 · 物理学 2022-05-25 R. Middei , A. Marinucci , V. Braito , S. Bianchi , B. De Marco , A. Luminari , G. Matt , E. Nardini , M. Perri , J. N. Reeves , F. Vagnetti

The star KIC 8462852 (Boyajian's Star) displays both fast dips of up to 20% on time scales of days, plus long-term secular fading by up to 19% on time scales from a year to a century. We report on CCD photometry of KIC 8462852 from 2015.75…

We present the results of $WBVR$ observations of the low-mass X-ray binary V1341 $\textrm{Cyg} = \textrm{Cyg}$ X--2. Our observations include a total of 2375 individual measurements in four bands on 478 nights in 1986-1992. We tied the…

太阳与恒星天体物理 · 物理学 2015-05-20 A. N. Sazonov

We report the discovery of a large number of short-period variable stars in the dwarf irregular galaxy NGC6822, based on deep time-series imaging carried out with the ESO Very Large Telescope. In particular, we found a modest population of…

天体物理学 · 物理学 2009-11-07 G. Clementini , E. V. Held , L. Baldacci , L. Rizzi

The behavior of the bright red supergiant, Betelgeuse, is described with results principally from the past 6 years. The review includes imaging, photometry, and spectroscopy to record the Great Dimming of 2019--2020. This event was followed…

太阳与恒星天体物理 · 物理学 2025-07-23 Andrea K. Dupree , Miguel Montargès