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相关论文: Three New Variable Stars in Indus

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We present the results of a photometric variability survey in the young open cluster Stock 14 and the surrounding fields. In total, we detected 103 variable stars of which 88 are new discoveries. We confirm short-period, low-amplitude light…

太阳与恒星天体物理 · 物理学 2013-10-01 D. Drobek , A. Pigulski , R. R. Shobbrook , A. Narwid

Results of the first two month of observations using the All Sky Automated Survey prototype camera are presented. More than 45 000 stars in 24 Selected Fields covering 140 sq. degrees were monitored a few times a night resulting in the…

天体物理学 · 物理学 2007-05-23 G. Pojmanski

By digitizing astronomical photographic plates one may extract full information stored on them, something that could not be practically achieved with classical analogue methods. We are developing algorithms for variable objects search using…

太阳与恒星天体物理 · 物理学 2014-03-24 Kirill Sokolovsky , Sergei Antipin , Daria Kolesnikova , Alexandr Lebedev , Nikolai Samus , Lyudmila Sat , Alexandra Zubareva

The results of the searching on the bases of GPS UKIDSS survey's data of dense compact stellar clusters in the vicinity of 20 YSOs with high and middle masses are presented. Totally we have revealed clusters in 13 areas. Around 5 objects…

太阳与恒星天体物理 · 物理学 2015-12-29 N. M. Azatyan , E. H. Nikoghosyan

I report on the discovery of two cataclysmic variables in the same field in Lyra originally identified from their magnitudes in USNO-B1.0 catalogue and Palomar images. The historical light curves were analyzed on 300+ photographic plates…

太阳与恒星天体物理 · 物理学 2011-07-20 D. V. Denisenko

We present ten years of new photometric monitoring of the light variability of five evolved stars with strong mid-infrared emission from surrounding dust. Three are known carbon-rich proto-planetary nebulae (PPNe) with F$-$G spectral types;…

太阳与恒星天体物理 · 物理学 2020-01-08 Bruce J. Hrivnak , Gary Henson , Todd C. Hillwig , Wenxian Lu , Brian W. Murphy , Ronald H. Kaitchuck

We present the results of a comprehensive search for stellar variability in the globular cluster 47 Tucanae. Using the Mount Stromlo 40-inch (1m) telescope at Siding Spring Observatory and a combined V+R filter, we have detected 100…

天体物理学 · 物理学 2010-02-18 David T F Weldrake , Penny D Sackett , Terry J Bridges , Kenneth C Freeman

We present a comprehensive survey of diffuse interstellar bands (DIBs) in $0.91-1.32\mu$m with a newly-developed near-infrared (NIR) spectrograph, WINERED, mounted on the Araki 1.3 m Telescope in Japan. We obtained high-resolution…

We present the discovery of 816 high amplitude infrared variable stars ($\Delta K_{\rm s} >$ 1 mag) in 119 deg$^2$ of the Galactic midplane covered by the Vista Variables in the Via Lactea (VVV) survey. Almost all are new discoveries and…

A radial velocity (RV) survey to detect central stars in binary systems was carried out between 2002 and 2004. De Marco et al. (2004) reported that 10 out of 11 monitored stars exhibited strong RV variability, but periods were not detected.…

天体物理学 · 物理学 2007-09-12 Orsola De Marco , S. Wortel , Howard E. Bond , Dianne Harmer

We report the first results of a study of variable point sources identified using multi-color time-series photometry from Sloan Digital Sky Survey (SDSS) Stripe 82 over a span of nearly 10 years (1998-2007). We construct a light-curve…

太阳与恒星天体物理 · 物理学 2014-11-20 Waqas A. Bhatti , Michael W. Richmond , Holland C. Ford , Larry D. Petro

We present a far-ultraviolet (FUV) study of the globular cluster M30 (NGC 7099). The images were obtained using the Advanced Camera for Surveys (ACS/SBC, F150LP, FUV) and the Wide Field Planetary Camera 2 (WFPC2, F300W, UV) on board the…

太阳与恒星天体物理 · 物理学 2022-04-22 Santana Mansfield , Andrea Dieball , Pavel Kroupa , Christian Knigge , David R. Zurek , Michael Shara , Knox S. Long

We present Cousins $R$ and $I$ band photometry of variable stars in a $\sim13'\times 13'$ region in the disk of M31 galaxy, obtained during 141 nights. Of the 26 Cepheid variables present in the region, two are newly discovered, 11 are…

天体物理学 · 物理学 2009-04-13 Y. C. Joshi , A. K. Pandey , D. Narasimha , R. Sagar , Y. Giraud-Hiraud

Intensive monitoring of low-extinction windows towards the galactic bulge has provided in the last years valuable information for studies about the dynamics, kinematics and formation history of this part of the galaxy, mainly by…

天体物理学 · 物理学 2016-08-15 T. P. Dominici , J. E. Horvath , G. A. Medina Tanco , R. Teixeira , P. Benevides-Soares

We present measurements of the periods, amplitudes, and types of 74 RR Lyrae stars in the globular cluster M15 derived from Nickel 1 m telescope observations conducted at LickObservatory in 2019 and 2020. Of these RR Lyrae stars, two were…

太阳与恒星天体物理 · 物理学 2021-01-13 Andrew M. Hoffman , Yukei S. Murakami , WeiKang Zheng , Benjamin E. Stahl , Alexei V. Filippenko

We present the results of a search for variable stars in the faint sparse globular cluster E3. We have found two variable stars: an SX Phe variable (V1) and a W UMa eclipsing binary (V2). We have applied period-luminosity and…

天体物理学 · 物理学 2008-11-26 B. J. Mochejska , J. Kaluzny , I. Thompson

We quantify the variability of faint unresolved optical sources using a catalog based on multiple SDSS imaging observations. The catalog covers SDSS Stripe 82, and contains 58 million photometric observations in the SDSS ugriz system for…

We have conducted a photometric survey of the globular cluster NGC 6397 in a search for variable stars. We obtained ~11h of time-resolved photometric images with one ne European Southern Observatory-Very Large Telescope using the FOcal…

太阳与恒星天体物理 · 物理学 2017-05-31 E. Martinazzi , S. O. Kepler , J. E. S. Costa

We investigate the infrared variability of carbon stars in the Large Magellanic Cloud (LMC). Our sample consists of 11,134 carbon stars identified in both visual and infrared bands. Among these, 1,184 objects are known Mira variables based…

太阳与恒星天体物理 · 物理学 2025-06-30 Kyung-Won Suh

We report here CCD $I$-band time-series photometry of a young (2$-$5 Myr) cluster NGC 2282 to identify and understand the variability of pre-main-sequence (PMS) stars. The $I$-band photometry, down to $\sim$ 20.5 mag, enables us to probe…

星系天体物理 · 物理学 2018-04-04 Somnath Dutta , Soumen Mondal , Santosh Joshi , Jessy Jose , Ramkrishna Das , Supriyo Ghosh
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