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相关论文: HD 69686: A Mysterious High Velocity B Star

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Aims. We study a sample of eight B[e] stars with uncertain evolutionary status to shed light on the origin of their circumstellar dust. Methods. We performed a diagnostic analysis on the spectral energy distribution beyond infrared…

太阳与恒星天体物理 · 物理学 2016-08-17 Chien-De Lee , W. P. Chen , S. Y. Liu

Small amounts of star formation in elliptical galaxies are suggested by several results: surprisingly young ages from optical line indices, cooling X-ray gas, and mid-IR dust emission. Such star formation has previously been difficult to…

宇宙学与河外天体物理 · 物理学 2015-06-05 H. Alyson Ford , Joel N. Bregman

We report the discovery of four rare debris disks with warm excesses around F-stars, significantly increasing the number of such systems known in the solar neighborhood. Three of the disks are consistent with the predictions of steady state…

太阳与恒星天体物理 · 物理学 2009-08-05 A. Moór , D. Apai , I. Pascucci , P. Ábrahám , C. Grady , Th. Henning , A. Juhász , Cs. Kiss , Á. Kóspál

Utilizing astrometric parameters sourced from \textit{Gaia} Data Release 3 and radial velocities obtained from various spectroscopic surveys, we identify 519 high-velocity stars (HiVels) with a total velocity in the Galactocentric restframe…

星系天体物理 · 物理学 2024-01-05 Jiwei Liao , Cuihua Du , Mingji Deng , Dashuang Ye , Hefan Li , Yang Huang , Jianrong Shi , Jun Ma

Very few examples are known of red supergiant runaways, all of them descending from the more massive O-type precursors, but none from the lower mass B-type precursors, although runaway statistics among B-type stars suggest that K-type…

太阳与恒星天体物理 · 物理学 2020-06-24 F. Comerón , F. Figueras

As Be stars are restricted to luminosity classes III-V, but early B-type stars are believed to evolve into supergiants, it is to be expected that the Be phenomenon disappears at some point in the evolution of a moderately massive star,…

天体物理学 · 物理学 2009-11-10 Ignacio Negueruela

The Sun-like star HD209458 harbors a close-in giant planet which transits across the star's disk, and thus allows an unprecedented access to the basic parameters of the planet, given a certain knowledge of the basic parameters of the star,…

天体物理学 · 物理学 2009-11-07 A. Cody , Dimitar D. Sasselov

In recent years several hypervelocity stars (HVSs) have been observed in the halo of our Galaxy. Such stars are thought to be ejected through dynamical interactions near the massive black hole (MBH) in the Galactic center. Three scenarios…

天体物理学 · 物理学 2008-12-18 Hagai B. Perets

Open clusters offer us the means to study stellar properties in samples with well-defined ages and initial chemical composition. Here we present a survey of projected rotational velocities for a large sample of mainly B-type stars in young…

天体物理学 · 物理学 2008-11-26 Wenjin Huang , Douglas R. Gies

Hyper-velocity stars (HVS) are enigmatic objects because they are travelling so fast that they escape from the Galaxy. Among hot subdwarfs, only one such star is known, the He-sdO US 708. The Hyper-MUCHFUSS collaboration provided additional…

太阳与恒星天体物理 · 物理学 2023-04-07 Ulrich Heber

Runaway stars are OB-type stars ejected from their birthplace with large peculiar velocities. The leading hypothesis addressed in their formation includes the supernova ejection mechanism and the dynamic ejection scenario. Identification of…

太阳与恒星天体物理 · 物理学 2024-05-09 Yanjun Guo , Luqian Wang , Chao Liu , You Wu , ZhanWen Han , XueFei Chen

Hills (1988) predicted that runaway stars could be accelerated to velocities larger than 1000 km/s by dynamical encounters with the supermassive black hole (SMBH) in the Galactic center. The recently discovered hypervelocity star SDSS…

天体物理学 · 物理学 2009-11-13 Alessia Gualandris , Simon Portegies Zwart , Michael Sipior

HD 8673 hosts a massive exoplanet in a highly eccentric orbit (e=0.723). Based on two epochs of speckle interferometry a previous publication identified a candidate stellar companion. We observed HD 8673 multiple times with the 10 m Keck II…

We measure the metallicity of the unusual hypervelocity star HE 0437-5439 from high resolution spectroscopy to be half-solar. We determine a spectral type of B2 IV-III for the star and derive an effective temperature Teff= 21,500 +/- 1,000…

天体物理学 · 物理学 2009-11-13 Alceste Z. Bonanos , Mercedes Lopez-Morales , Ian Hunter , Robert S. I. Ryans

We present the re-detection of a compact source in the face-on protoplanetary disc surrounding HD 169142, using VLT/SPHERE data in YJH bands. The source is found at a separation of 0.''319 ($\sim$37 au) from the star. Three lines of…

地球与行星天体物理 · 物理学 2023-03-15 Iain Hammond , Valentin Christiaens , Daniel J. Price , Claudia Toci , Christophe Pinte , Sandrine Juillard , Himanshi Garg

We define an enhanced spectral classification scheme for M dwarf stars, and use it to derive spectral classification of 104 northern stars with proper motions larger than 0.5"/yr which we discovered in a survey of high proper motion stars…

天体物理学 · 物理学 2009-11-07 Sebastien Lepine , R. Michael Rich , Michael M. Shara

We present multiple epochs of H-alpha spectroscopy for 47 members of the open cluster NGC 3766 to investigate the long term variability of its Be stars. Sixteen of the stars in this sample are Be stars, including one new discovery. Of…

We use new Gaia measurements to explore the origin of the highest velocity stars in the Hypervelocity Star Survey. The measurements reveal a clear pattern in the B-type stars. Halo stars dominate the sample at speeds about 100 km/s below…

太阳与恒星天体物理 · 物理学 2018-10-17 Warren R. Brown , Mario G. Lattanzi , Scott J. Kenyon , Margaret J. Geller

We present the discovery of a previously unknown very nearby star - LHS 2090 at a distance of only d=6 pc. In order to find nearby (i.e. d < 25 pc) red dwarfs, we re-identified high proper motion stars ($\mu >$ 0.18 arcsec/yr) from the NLTT…

天体物理学 · 物理学 2016-08-30 R. -D. Scholz , H. Meusinger , H. Jahreiß

High-resolution spectroscopic observations were taken of 29 extended main sequence turn-off (eMSTO) stars in the young ($\sim$200 Myr) LMC cluster, NGC 1866 using the Michigan/Magellan Fiber System and MSpec spectrograph on the…