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相关论文: Oxygen rich cool stars in the Cepheus region, New …

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We analyzed the light curves of 165 AGB variables, mostly Miras, in the sky area centered between M16 and M17 (l=16, b=0), using the OGLE GVS database in the I_C band. Comparison with the published light curves, derived about 50 years…

太阳与恒星天体物理 · 物理学 2022-06-08 Roberto Nesci , Igor Soszyński , Taavi Tuvikene

HIPPARCOS astrometric and kinematical data of oxygen-rich Mira variables are used to calibrate absolute near-infrared magnitudes and kinematic parameters. Two sets of near-infrared magnitudes compiled from different authors are used:…

天体物理学 · 物理学 2007-05-23 R. Alvarez , M-O. Mennessier , D. Barthes , X. luri , J. A. Mattei

For nine Mira-type stars (o Cet, R Leo, S Car, U Her, X Oph, R Aql, RR Aql, S Ori, S Scl,) and one semi-regular star (L2 Pup), the mean light curves have been obtained. The initial values of the brightness (observations) were fitted by a…

太阳与恒星天体物理 · 物理学 2017-01-18 L. S. Kudashkina

We use the OGLE-II and OGLE-III data in conjunction with the 2MASS near-infrared (NIR) photometry to identify and study Miras and Semiregular Variables (SRVs) in the Large Magellanic Cloud. We found in total 3221 variables of both types,…

Near-infrared, JHKL, photometry of 239 Galactic carbon-rich variable stars is presented and discussed. From these and published data the stars were classified as Mira or non-Mira variables and amplitudes and pulsation periods, ranging from…

天体物理学 · 物理学 2009-11-11 Patricia A. Whitelock , Michael W. Feast , Freddy Marang , M. A. T. Groenewegen

We present the first cross-identifications of sources in the near-infrared DENIS survey and in the micro-lensing EROS survey in a field of about 0.5 square degrees around the optical center (OC) of the Large Magellanic Cloud. We analyze the…

天体物理学 · 物理学 2009-11-07 M-R. L. Cioni , J-B. Marquette , C. Loup , M. Azzopardi , H. J. Habing , T. Lasserre , E. Lesquoy

The absolute K magnitudes and kinematic parameters of about 350 oxygen-rich Long-Period Variable stars are calibrated, by means of an up-to-date maximum-likelihood method, using Hipparcos parallaxes and proper motions together with radial…

天体物理学 · 物理学 2009-10-31 D. Barthes , X. Luri , R. Alvarez , M. O. Mennessier

We report on spectroscopic and photometric observations of the S-type Mira V667 Cas and the carbon star Mira OR Cep recorded during one pulsation cycle of each star in 2022. Spectra are calibrated in absolute flux using concurrent…

太阳与恒星天体物理 · 物理学 2024-07-03 David Boyd

We analyze sparsely-sampled near-infrared (JHKs) light curves of a sample of 1781 Mira variable candidates in M33, originally discovered using I-band time-series observations. We extend our single-band semi-parametric Gaussian process…

太阳与恒星天体物理 · 物理学 2018-08-29 Wenlong Yuan , Lucas M. Macri , Atefeh Javadi , Zhenfeng Lin , Jianhua Z. Huang

King, Modjaz, & Li (1999) discovered Nova 1999 in IC1613 at Lick Observatory. Both Fugazza et al. (2000) and Borissova et al. (2000) questioned this classification, because they were able to detect the star on images obtained in previous…

天体物理学 · 物理学 2009-11-07 R. Kurtev , L. Georgiev , J. Borissova , W. D. Li , A. V. Filippenko , R. R. Treffers

K-band spectra of young stellar candidates in four southern hemisphere clusters have been obtained with the near-infrared spectrograph GNIRS in Gemini South. The clusters are associated with IRAS sources that have colours characteristic of…

天体物理学 · 物理学 2009-11-13 A. Roman-Lopes , Z. Abraham , R. Ortiz , A. Rodrigues-Ardila

Several values for the magnitudes and spectral types of the components of the binary Mira X Ophiuchi have been published in the literature over the last century. Analysis of new photometry and spectroscopy of the star between 2016 May and…

太阳与恒星天体物理 · 物理学 2018-04-04 David Boyd

We present optical $I$-band light curves of the stars towards a star-forming region Cygnus OB7 from 17 nights photometric observations. The light curves are generated from a total of 381 image frames with very good photometric precision.…

太阳与恒星天体物理 · 物理学 2019-05-29 Somnath Dutta , Soumen Mondal , Santosh Joshi , Ramkrishna Das

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 report the discovery of two Mira variable stars (Miras) toward the Sextans dwarf spheroidal (dSph) galaxy. We performed optical long-term monitoring observations for two red stars in the Sextans dSph. The light curves of both stars in…

星系天体物理 · 物理学 2015-06-11 T. Sakamoto , N. Matsunaga , T. Hasegawa , Y. Nakada

We present initial results of the first panoramic search for high-amplitude near-infrared variability in the Galactic Plane. We analyse the widely separated two-epoch K-band photometry in the 5th and 7th data releases of the UKIDSS Galactic…

We present the results of a massive variability search based on a photometric survey of a six square degree region along the Galactic plane at ($l = 305^\circ$, $b = -0.8^\circ$) and ($l = 330^\circ$, $b = -2.5^\circ$). This survey was…

We present a sample of 4,132 Mira-like variables (red variables with long periods and high amplitudes) in the Kilodegree Extremely Little Telescope (KELT) survey. Of these, 814 are new detections. We used 2MASS colors to identify candidate…

This project is a massive near-infrared (NIR) search for variable stars in highly reddened and obscured open cluster (OC) fields projected on regions of the Galactic bulge and disk. The search is performed using photometric NIR data in the…

In this paper we present the fourth part of the photometric data from the 9x9 deg ASAS camera monitoring the whole southern hemisphere in V-band. Preliminary list (based on observations obtained since January 2001) of variable stars located…

天体物理学 · 物理学 2007-05-23 G. Pojmanski , Gracjan Maciejewski
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