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相关论文: Spectral Type and Radial Velocity Variations in Th…

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Slow-rotating evolved stars frequently exhibit radial velocity (RV) variations on annual timescales, complicated by instrumental systematics and aliasing in the one-year regime. Here we investigate the origin of the near-yearly periodicity…

Spectroscopic and photometric variability is widespread among O-type supergiants. It is linked to various phenomena affecting the star and its circumstellar environment, thereby providing direct information concerning them. To investigate…

太阳与恒星天体物理 · 物理学 2025-08-05 Gregor Rauw , Yaël Nazé , Charles-Antoine Gilon

Stars exhibit a bewildering variety of rapidly variable behaviors ranging from explosive magnetic flares to stochastically changing accretion to periodic pulsations or rotation. The principal Rubin Observatory Legacy Survey of Space and…

太阳与恒星天体物理 · 物理学 2023-08-02 Eric D. Feigelson , Federica B. Bianco , Rosaria Bonito

The long-time photometric surveys in a few young open clusters allowed to identify the light variability in stars located on the HR diagram between the well defined $\delta$ Scuti variables and Slowly Pulsating B-type stars. Several objects…

太阳与恒星天体物理 · 物理学 2017-11-08 Jadwiga Daszynska-Daszkiewicz , Przemyslaw Walczak , Alexey Pamyatnykh

We report CCD $V$ and $I$ time-series photometry of the globular cluster NGC 6333 (M9). The technique of difference image analysis has been used, which enables photometric precision better than 0.05 mag for stars brighter than $V \sim 19.0$…

A majority part of magnetic chemically peculiar (mCP) stars of the upper main sequence exhibits strictly periodic light, magnetic, radio, and spectral variations that can be fully explained by the model of a rigidly rotating main-sequence…

太阳与恒星天体物理 · 物理学 2017-02-27 Zdeněk Mikulášek

Red giants are evolved stars which exhibit solar-like oscillations. Although a multitude of stars have been observed with space telescopes, only a handful of red-giant stars were targets of spectroscopic asteroseismic observing projects. We…

In this paper we review the observational data for OB stars in the SMC concentrating on those aspects of their spectra which provide information on processes which may strongly influence their evolution, namely mass-loss, rotational mixing…

天体物理学 · 物理学 2007-05-23 D. J. Lennon , C. J. Evans , C. Trundle

We discuss moderate resolution spectra, multicolor photometry, and light curves of thirty-one of the most luminous stars and variables in the giant spiral M101. The majority are intermediate A to F-type supergiants. We present new…

太阳与恒星天体物理 · 物理学 2015-06-23 Skyler H. Grammer , Roberta M. Humphreys , Jill Gerke

We present the results of a 5.5-year CCD photometric campaign that monitored 261 bright, southern, semi-regular variables with relatively precise Hipparcos parallaxes. The data are supplemented with independent photoelectric observations of…

太阳与恒星天体物理 · 物理学 2015-05-14 V. Tabur , T. R. Bedding , L. L. Kiss , T. T. Moon , B. Szeidl , H. Kjeldsen

We present spectroscopic rotation velocities (v sin i) for 56 M dwarf stars using high resolution HET HRS red spectroscopy. In addition we have also determined photometric effective temperatures, masses and metallicities ([Fe/H]) for some…

太阳与恒星天体物理 · 物理学 2015-05-14 J S Jenkins , L W Ramsey , H R A Jones , Y Pavlenko , J Gallardo , J R Barnes , D J Pinfield

We present new results from follow-up time-resolved spectroscopy of radial velocity variable hot subdwarfs from the SPY project. Medium resolution spectra were taken at the ESO NTT. Preliminary orbital solutions are presented for three…

天体物理学 · 物理学 2008-04-09 S. Geier , U. Heber , R. Napiwotzki

We present results of a variability search in the intermediate-age open cluster NGC 6866 from 29 nights over two observing seasons. We find 28 periodic variables, of which 19 are newly identified. The periods of these variables, which have…

太阳与恒星天体物理 · 物理学 2015-05-30 Yogesh C. Joshi , Santosh Joshi , Brijesh Kumar , Soumen Mondal , L. A. Balona

For 6 years the Convection, Rotation, and Planetary Transits (CoRoT) space mission has acquired photometric data from more than one hundred thousand point sources towards and directly opposite from the inner and outer regions of the Galaxy.…

Cataclysmic variables are among the photometrically most unstable stars in the zoo of stellar objects, exhibiting light variations on all time-scales between millennia and seconds. The literature is full of reports on variable phenomena…

太阳与恒星天体物理 · 物理学 2020-02-17 Albert Bruch

We present new radial velocities, improved pulsation periods and reference epoch s of 11 field RR Lyrae ab-type variables: AS Vir, BS Aps, CD Vel, DT Hya, RV Oct, TY Gru, UV Oct, V1645 Sgr, WY Ant, XZ Aps and Z Mic. This study is based on…

太阳与恒星天体物理 · 物理学 2015-05-27 Bi-Qing For , George W. Preston , Christopher Sneden

We report the detection of velocity variations in the pulsating sdB star, PG 1605+072. Oscillations are detected at the same frequencies found from photometry and have amplitudes of up to 14 km/s for H$\beta$. The strongest oscillation…

We present time-series photometry of 11 hypervelocity stars (HVSs) to constrain their nature. Known HVSs are mostly late-B spectral type objects that may be either main-sequence (MS) or evolved blue horizontal branch (BHB) stars.…

星系天体物理 · 物理学 2013-02-11 Idan Ginsburg , Warren R. Brown , Gary A. Wegner

Multiple radial velocity observations have been obtained for a large sample of local field subdwarf B (sdB) stars over a period of two years. SdB stars appear to fall into three distinct groups based on their kinematic and spectroscopic…

天体物理学 · 物理学 2007-05-23 Rex A. Saffer , Elizabeth M. Green , Timothy P. Bowers

Results of a search for variable stars in the central region of the globular cluster M13 are presented. Prior to this study, 36 variable and suspected variable stars were known in this cluster (Osborn 2000; Clement et al. 2001). Of these…

天体物理学 · 物理学 2009-11-07 G. Kopacki , Z. Kolaczkowski , A. Pigulski