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相关论文: Spatially resolved imaging spectroscopy of T Tauri

200 篇论文

We report the results of a spectroscopic survey of 20 close T Tauri binaries in the Taurus-Auriga dark cloud where the separations between primaries and their secondaries are less than the typical size of a circumstellar disk around a young…

天体物理学 · 物理学 2009-11-07 Patrick Hartigan , Scott Kenyon

We have analyzed photometric and spectroscopic data of a sample of 14 spatially resolved pre-main-sequence binaries (separations 0.6" to 1.7") in the nearby (150 pc) low-mass star-forming regions of Chamaeleon, Lupus, and rho Ophiuchi. The…

天体物理学 · 物理学 2007-05-23 Wolfgang Brandner , Hans Zinnecker

We detect near-infrared H2 emission in DG Tau using the Infrared Camera and Spectrograph (IRCS) on the 8.2-m SUBARU telescope. The spectra obtained along the jet axis show that the centroidal position of the 1-0 S(1) emission is offset by…

天体物理学 · 物理学 2009-11-10 M. Takami , A. Chrysostomou , T. P. Ray , C. Davis , W. R. F. Dent , J. Bailey , M. Tamura , H. Terada

We present 2.0-2.4micron integral field spectroscopy at adaptive optics spatial resolution (~0.''1) obtained with the Near-infrared Integral Field Spectrograph (NIFS) at Gemini North Observatory of six Classical T Tauri stars: T Tau, DG…

天体物理学 · 物理学 2009-11-13 Tracy L. Beck , Peter J. McGregor , Michihiro Takami , Tae-Soo Pyo

In accreting young stars one of the prominent spectral features in the near infrared is the Paschen and Brackett series in emission. We examine hydrogen line ratios for 16 classical T Tauri stars from SpeX spectra and and assess the trends…

太阳与恒星天体物理 · 物理学 2015-06-17 Suzan Edwards , John Kwan , William Fischer , Lynne Hillenbrand , Kimberly Finn , Kristina Fedorenko , Wanda Feng

Context : The properties of the inner disks of bright Herbig AeBe stars have been studied with near infrared (NIR) interferometry and high resolution spectroscopy. The continuum and a few molecular gas species have been studied close to the…

We have analyzed GHRS data of eight Classical T Tauri stars (CTTSs) and one Weak T Tauri star (WTTS). The GHRS data consist of an spectral range 40 A wide centered on 2800 A. For 4 of the CTTS we have nearly simultaneous optical…

We present multi-epoch optical and near-infrared (NIR) photometry and spectroscopy of the spectroscopic binary T Tauri star DQ Tau. The photometric monitoring, obtained using SMARTS ANDICAM, recovers the previously-seen correlation between…

太阳与恒星天体物理 · 物理学 2019-05-29 James Muzerolle , Kevin Flaherty , Zoltan Balog , Tracy Beck , Robert Gutermuth

We have analyzed GHRS data of eight CTTS and one WTTS. The GHRS data consists of spectral ranges 40 A wide centered on 1345, 1400, 1497, 1550, and 1900 A. These UV spectra show strong SiIV, and CIV emission, and large quantities of sharp…

天体物理学 · 物理学 2009-11-07 D. R. Ardila , G. Basri , F. M. Walter , J. A. Valenti , C. M. Johns-Krull

We present spatially-resolved X-ray observations of the binary T Tauri star system V710 Tau. Using Chandra's Advanced CCD Imaging Spectrometer (ACIS), we imaged this 3.2'' separation binary system, consisting of a classical T Tauri star,…

天体物理学 · 物理学 2009-11-13 Sonali J. Shukla , David A. Weintraub , Joel H. Kastner

Context. In multiple pre-main-sequence systems the lifetime of circumstellar disks appears to be shorter than around single stars, and the actual dissipation process may depend on the binary parameters of the systems. Aims. We report high…

太阳与恒星天体物理 · 物理学 2017-07-12 Gergely Csépány , Mario van den Ancker , Péter Ábrahám , Rainer Köhler , Wolfgang Brandner , Felix Hormuth , Hector Hiss

We present an infrared imaging study of the low-mass pre-main sequence binary system Haro 6-10. This system is one of a handful in which the optically-visible primary has the characteristics of a normal T Tauri star, while the secondary is…

天体物理学 · 物理学 2009-10-31 C. D. Koresko , G. A. Blake , M. E. Brown , A. I. Sargent , D. W. Koerner

We construct detailed vertical structure models of irradiated accretion disks around T Tauri stars with interstellar medium dust uniformly mixed with gas. The dependence of the structure and emission properties on mass accretion rate,…

天体物理学 · 物理学 2009-10-31 Paola D'Alessio , Nuria Calvet , Lee Hartmann , Susana Lizano , Jorge Canto

The optical star in the T Tauri triple system is the prototype of young sun-like stars in our galaxy. This complex and dynamic system has evidence for misaligned disks and outflows, and molecular material in a circumbinary ring that…

太阳与恒星天体物理 · 物理学 2025-01-14 Tracy L. Beck

Aims: We investigate the structure of the circumstellar disk of the T Tauri star S CrA N and test whether the observations agree with the standard picture proposed for Herbig Ae stars. Methods: Our observations were carried out with the…

太阳与恒星天体物理 · 物理学 2014-03-19 J. Vural , A. Kreplin , S. Kraus , G. Weigelt , T. Driebe , M. Benisty , M. Dugué , F. Massi , J. -L. Monin , M. Vannier

Most of our knowledge about star formation is based on studies of low-mass stars, whereas very little is known about the properties of the circumstellar material around young and embedded intermidiate-mass T Tauri stars (IMTTSs). We present…

FN Tau is a rare example of very low-mass T Tauri stars that exhibits a spatially resolved nebulosity in near-infrared scattering light. To directly derive the parameters of a circumstellar disk around FN Tau, observations of dust continuum…

星系天体物理 · 物理学 2015-05-18 Munetake Momose , Nagayoshi Ohashi , Tomoyuki Kudo , Motohide Tamura , Yoshimi Kitamura

The results of a spectroscopic survey of H alpha emission line stars associated with fourteen bright rimmed clouds are presented. Slit-less optical spectroscopy was carried out with the Inter University Centre for Astronomy and Astrophysics…

太阳与恒星天体物理 · 物理学 2020-06-02 Kensuke Hosoya , Yoichi Itoh , Yumiko Oasa , Ranjan Gupta , Asoke Kumar Sen

Using NASA IRTF SpeX data from 0.8 to 4.5 $\mu$m, we determine self-consistently the stellar properties and excess emission above the photosphere for a sample of classical T Tauri stars (CTTS) in the Taurus molecular cloud with varying…

太阳与恒星天体物理 · 物理学 2015-06-15 M. K. McClure , N. Calvet , C. Espaillat , L. Hartmann , J. Hernandez , L. Ingleby , K. L. Luhman , P. D'Alessio , B. Sargent