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The study of ionized gas morphology and kinematics in nine eXtremely Metal-Deficient (XMD) galaxies with the scanning Fabry-Perot interferometer on the SAO 6-m telescope is presented. Some of these very rare objects (with currently known…

宇宙学与河外天体物理 · 物理学 2015-05-18 A. V. Moiseev , S. A. Pustilnik , A. Y. Kniazev

We report the discovery of a nearby M5.0V dwarf at 24.6 pc, SCR 1848-6855, that is orbited by an unusual companion causing an astrometric perturbation of more than 200 milli-arcseconds. This is by far the largest perturbation found to date…

太阳与恒星天体物理 · 物理学 2015-06-17 Wei-Chun Jao , Todd J. Henry , John P. Subasavage , Jennifer G. Winters , Douglas R. Gies , Adric R. Riedel , Philip A. Ianna

We report the detection of a double planetary system around the evolved intermediate-mass star HD 47366 from precise radial-velocity measurements at Okayama Astrophysical Observatory, Xinglong Station, and Australian Astronomical…

After the discovery of a substellar companion to the hot subdwarf HD 149382, we have started a radial velocity search for similar objects around other bright sdB stars using the Anglo-Australian Telescope. Our aim is to test the hypothesis…

地球与行星天体物理 · 物理学 2015-05-27 S. J. O'Toole , U. Heber , S. Geier , L. Classen , O. De Marco

Massive B-type stars with strong magnetic fields and fast rotation are very rare and provide a mystery for theories of both star formation and magnetic field evolution. Only two such stars, called sigma Ori E analogs, were previously known.…

太阳与恒星天体物理 · 物理学 2015-06-03 S. Hubrig , M. Schöller , L. Fossati , T. Morel , N. Castro , L. M. Oskinova , N. Przybilla , S. S. Eikenberry , M. F. Nieva , N. Langer

Using a sample of 43 bright (V<16.1, distance <13 kpc) RR Lyrae stars (RRLS) from the QUEST survey with spectroscopic radial velocities and metallicities, we find that several separate halo substructures contribute to the Virgo overdensity…

天体物理学 · 物理学 2011-08-31 A. Katherina Vivas , Yara Jaffe , Robert Zinn , Rebeccah Winnick , Sonia Duffau , Cecilia Mateu

We report the discovery of a bright (V ~ 13.7), extremely low-mass white dwarf in a close double degenerate system. We originally selected GALEX J171708.5+675712 for spectroscopic follow-up among a group of white dwarf candidates in an…

太阳与恒星天体物理 · 物理学 2011-08-02 S. Vennes , J. R. Thorstensen , A. Kawka , P. Nemeth , J. N. Skinner , A. Pigulski , M. Steslicki , Z. Kolaczkowski , P. Srodka

Little Red Dots (LRDs) are compact, red sources discovered by JWST at high redshift ($z \gtrsim 4$), marked by distinctive "V-shaped" spectral energy distributions (SEDs) and often interpreted as rapidly accreting AGNs. Their evolution…

In this paper, we report 591 high velocity star candidates (HiVelSCs) selected from over 10 million spectra of the data release seven (DR7) of the Large Sky Area Multi-object Fiber Spectroscopic Telescope and the second Gaia data release,…

We report the discovery of an unusually red brown dwarf found in a search for high proper motion objects using WISE and 2MASS data. WISEP J004701.06+680352.1 is moving at 0.44$ arcsec/yr and lies relatively close to the Galactic Plane…

Observations made using TESS revealed a sample of low mass stars which show a periodic modulation on a period $<0.2$~d. Surprisingly many of these Ultra Fast Rotating (UFR) stars showed no evidence of flare activity which would be expected…

太阳与恒星天体物理 · 物理学 2022-02-23 Gavin Ramsay , Pasi Hakala , J. Gerry Doyle , Lauren Doyle , Stefano Bagnulo

We report the detection of a pair of dwarf galaxies at $z\!=\!0.30$ which may be in the early stages of an interaction. Both galaxies have stellar masses of $<10^{9}M_\odot$, and display a projected separation of $\sim\!29$kpc and a…

Abridged: We report the discovery of two, new, rare, wide, double-degenerate binaries that each contain a magnetic and a non-magnetic star. The components of SDSSJ092646.88+132134.5 + J092647.00+132138.4 and SDSSJ150746.48+521002.1 +…

Masses for 664 single-lined hot subdwarf stars identified in LAMOST were calculated by comparing synthetic fluxes from spectral energy distribution (SED) with observed fluxes from virtual observatory service. Three groups of hot subdwarf…

太阳与恒星天体物理 · 物理学 2023-08-16 Zhenxin Lei , Ruijie He , Peter Nemeth , Xuan Zou , Huaping Xiao , Yong Yang , Jingkun Zhao

We present a study of the evolutionary state of a few lithium-rich giant stars based on the Gaia DR2 parallaxes and photometry. We also investigate the chromospheric activity, the presence of a surface magnetic field, and the radial…

太阳与恒星天体物理 · 物理学 2020-09-09 B. F. O. Gonçalves , J. S. da Costa , L. de Almeida , M. Castro , J. -D. do Nascimento

Using K2 data, we have identified 23 very low mass members of the $\rho$ Oph and Upper Scorpius star-forming region as having periodic photometric variability not easily explained by well-established physical mechanisms such as star spots,…

The redshift range from 2.2 to 3, is known as the 'redshift desert' of quasars because quasars with redshift in this range have similar optical colors as normal stars and are thus difficult to be found in optical sky surveys. A quasar…

We have examined the relationship between rotation and activity in 14 late-type (M6-M7) M dwarfs, using high resolution spectra taken at the W.M. Keck Observatory and flux-calibrated spectra from the Sloan Digital Sky Survey. Most were…

天体物理学 · 物理学 2011-02-11 Andrew A. West , Gibor Basri

We report high precision, high cadence photometric measurements of the star HD 209458, which is known from radial velocity measurements to have a planetary mass companion in a close orbit. We detect two separate transit events at times that…

天体物理学 · 物理学 2009-10-31 David Charbonneau , Timothy M. Brown , David W. Latham , Michel Mayor

In Data Release 9 of LAMOST, we present measurements of v sin i for a total of 121,698 stars measured using the Medium Resolution Spectrograph (MRS) and 80,108 stars using the Low Resolution Spectrograph (LRS). These values were obtained…

太阳与恒星天体物理 · 物理学 2024-01-09 Fang Zuo , A-Li Luo , Bing Du , Yinbi Li , Hugh R. A. Jones , Yi-han Song , Xiao Kong , Yan-xin Guo