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相关论文: Spectral Variability of the Star HD 141569A

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Using the HiVIS spectropolarimeter built for the Haleakala 3.7m AEOS telescope, we have obtained a large number of high precision spectropolarimetrc observations (284) of Herbig AeBe stars collected over 53 nights totaling more than 300…

天体物理学 · 物理学 2009-11-13 D. M. Harrington , J. R. Kuhn

The more massive counterparts of T Tauri stars, Herbig Ae/Be stars, are known to vary in a complex way with no variability mechanism clearly identified. We attempt to characterize the optical variability of HD~37806 (MWC 120) on time scales…

太阳与恒星天体物理 · 物理学 2015-05-19 S. M. Rucinski , K. Zwintz , M. Hareter , G. Pojmanski , R. Kuschnig , J. M. Matthews , D. B. Guenther , A. F. J. Moffat , D. Sasselov , W. W. Weiss

Despite of the importance of magnetic fields for the full understanding of the properties of accreting Herbig Ae/Be stars, these fields have scarcely been studied over the rotation cycle until now. One reason for the paucity of such…

太阳与恒星天体物理 · 物理学 2015-05-20 S. Hubrig , Z. Mikulasek , J. F. Gonzalez , M. Schoeller , I. Ilyin , M. Cure , M. Zejda , C. R. Cowley , V. G. Elkin , M. A. Pogodin , R. V. Yudin

We search for periodic variations in the radial velocity of the young Herbig star HD 135344B with the aim to determine a rotation period. We analyzed 44 high-resolution optical spectra taken over a time range of 151 days. The spectra were…

太阳与恒星天体物理 · 物理学 2015-05-27 André Müller , Mario van den Ancker , Ralf Launhardt , Jörg-Uwe Pott , Davide Fedele , Thomas Henning

We present Halpha spectropolarimetry observations of a sample of 23 Herbig Ae/Be stars. A change in the linear polarisation across Halpha is detected in a large fraction of the objects, which indicates that the regions around Herbig stars…

天体物理学 · 物理学 2009-11-07 Jorick S. Vink , Janet E. Drew , Tim J. Harries , Rene D. Oudmaijer

We report on low resolution (R~3000) spectropolarimetry of the A0 supergiant star HD 92207. This star is well-known for significant spectral variability. The source was observed on seven different nights spanning approximately 3 months in…

天体物理学 · 物理学 2009-11-13 R Ignace , S Hubrig , M Scholler

Massive stars continuously enrich the surrounding interstellar medium by supplying it with stellar material driven by their powerful winds. B supergiant stars (BSGs) in particular are a type of massive star characterized by strong winds and…

太阳与恒星天体物理 · 物理学 2026-05-29 J. Chamoun-Contreras , C. Arcos , N. Machuca , C. E. Perez-Ramirez , L. S. Cidale , M. Curé , I. Araya , D. Turis-Gallo , M. Hadjara

We analysed 337 multi-epoch optical spectra of 38 Herbig Ae/Be (HAeBe) stars to gain insights into the variability behaviour of the circumstellar (CS) atomic gas. Equivalent widths (EWs) and line fluxes of the Halpha, [OI]6300, HeI5876 and…

太阳与恒星天体物理 · 物理学 2011-03-29 I. Mendigutía , C. Eiroa , B. Montesinos , A. Mora , R. D. Oudmaijer , B. Merín , G. Meeus

We analyse spectroscopic observations of the B[e] star HD 50138 (MWC 158, V743 Mon, or IRAS 06491-0654), a member of the FS CMa group, obtained over the last twenty years. Four different epochs are identified in the observational data,…

Chemically peculiar stars present spectral and photometric variability with a single period. In the oblique rotator model, the non homogeneous distribution of elements on the stellar surface is at the origin of the observed variations. As…

天体物理学 · 物理学 2017-03-22 G. Catanzaro , F. Leone , F. A. Catalano

Aims. We attempt to determine if a dependency on spectral subtype or vsini exists for stars undergoing phase-changes between B and Be states, as well as for those stars exhibiting variability in H{\alpha} emission. Methods. We analyse the…

太阳与恒星天体物理 · 物理学 2015-06-15 R. M. Barnsley , I. A. Steele

HD 141569 is a Herbig Ae/Be star that straddles the boundary between the transition disks and debris disks. It is a low dust mass disk that reveals numerous structural elements (e.g. gaps and rings) that may point to young planets. It also…

太阳与恒星天体物理 · 物理学 2021-12-16 Stanley K. Jensen , Sean D. Brittain , Joan R. Najita , John S. Carr

We obtained high-resolution, high signal-to-noise UVES and a few lower quality HARPS spectra revealing the presence of resolved magnetically split lines. HD101412 is the first Herbig Ae star for which the rotational Doppler effect was found…

太阳与恒星天体物理 · 物理学 2015-05-18 S. Hubrig , M. Schoeller , I. Savanov , J. F. Gonzalez , C. R. Cowley , O. Schuetz , R. Arlt , G. Ruediger

The polarization of light across individual spectral lines contains information about the circumstellar environment on very small spatial scales. We have obtained a large number of high precision, high resolution spectropolarimetric…

天体物理学 · 物理学 2009-11-13 D. M. Harrington , J. R. Kuhn

The Herbig Ae star HD 169142 is known to have a gaseous disk with a large inner hole, and also a photometrically variable inner dust component in the sub-au region. Following up our previous analysis, we further studied the temporal…

An analysis of solid-state features in infrared spectra of 46 Herbig Ae/Be stars is presented. The presence of solid-state emission bands is compared to other indicators of circumstellar material, such as Halpha emission, optical…

天体物理学 · 物理学 2007-05-23 M. E. van den Ancker

We have spectroscopically monitored the galactic Luminous Blue Variable HD 160529 and obtained an extensive high-resolution data set that covers the years 1991 to 2002. During this period, the star evolved from an extended photometric…

We present the very first analysis of the spectroscopic variability of the three rapidly rotating Oef stars HD192281 (O5(ef)), HD14442 (O5.5ef) and HD14434 (O6.5(ef)). Radial velocities of the HeII lambda 4541 line reveal no evidence of…

天体物理学 · 物理学 2009-11-10 M. De Becker , G. Rauw

We present thirteen epochs of near-infrared (0.8-5 micron) spectroscopic observations of the pre-transitional, "gapped" disk system in SAO 206462 (=HD 135344B). In all, six gas emission lines (including Br gamma, Pa beta, and the 0.8446…

We present results of a study of the variability of the marginal Am star HD\,176843 observed in the {\it Kepler} field. {\it Kepler} photometry and ground-based spectroscopy are used to investigate the light variations of the star.…

太阳与恒星天体物理 · 物理学 2019-04-02 C. Ulusoy , I. Stateva , B. Ulaş , F. Aliçavuş , I. Kh. Iliev , M. Napetova , E. Kaygan
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