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Related papers: High-resolution Spectroscopy of [Ne II] Emission f…

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We present new results of [Fe II] 1.644-micron spectroscopy toward the jets from HL Tau and RW Aur carried out with the Subaru Telescope combined with the adaptive optics system. We observed the regions within 2" - 3" from the stars with…

We present new continuum and line observations, along with modelling, of the faint (6-8) Myr old T Tauri star ET Cha belonging to the eta Chamaeleontis cluster. We have acquired HERSCHEL/PACS photometric fluxes at 70 mic and 160 mic, as…

We explore the kinematics of the stars, ionized gas, and warm molecular gas in the Seyfert 2 galaxy Mrk~3 (UGC~3426) on nuclear and galactic scales with {\it Gemini} Near-Infrared Field Spectrograph (NIFS) observations, previous {\it Hubble…

We present high-resolution Chandra HETGS X-ray spectra of the classical T Tauri star SU Aur. The quiescent X-ray emission is dominated by a 20-40 MK plasma, which contrasts strongly with the cool 3 MK plasma dominating the X-ray emission of…

Astrophysics · Physics 2007-05-23 K. Smith , M. Audard , M. Guedel , S. Skinner , R. Pallavicini

We present new [Ne II] (12.8 micron) IRTF/TEXES observations of the Galactic Center HII regions H1 and H2, which are at a projected distance of ~11 pc from the center of the Galaxy. The new observations allow to map the radial velocity…

Spitzer Space Telescope infrared measurements are presented for 24 members of the TW Hydrae association (TWA). High signal-to-noise 24-micron (um) photometry is presented for all of these stars, including 20 stars that were not detected by…

Astrophysics · Physics 2009-11-11 F. J. Low , P. S. Smith , M. Werner , C. Chen , V. Krause , M. Jura , D. C. Hines

Using the speckle camera SHARP at the 3.5m ESO NTT, K\"ohler and collaborators found an object ~3.5 mag fainter in K only 1.3" north-east of the T Tauri star [MR81] Ha 17 in the Corona Australis (CrA) star-forming region, which could be…

Solar and Stellar Astrophysics · Physics 2009-11-13 R. Neuhaeuser , S. Kraemer , M. Mugrauer , R. Koehler , T. O. B. Schmidt , M. Ammler-von Eiff , J. Alves , S. Fiedler , N. Vogt

We have obtained three long-slit, far UV spectra of the pre-main sequence system T Tauri. These HST/STIS spectra show a strong and variable on-source spectrum composed of both fluoresced H_2 and stellar chromospheric lines. Extended H_2…

Aims: We search for PAH features towards T Tauri stars and compare them with surveys of Herbig Ae/Be stars. The presence and strength of the PAH features are interpreted with disk radiative transfer models exploring the PAH feature…

We investigated an isolated, globule-shaped object (0.37x0.11 pc), located near the centre of the Cygnus OB2 cluster and named proplyd #7 in optical observations. The source can be a massive star (with or without disc) with a HII region or…

We present a comprehensive set of spatially resolved, integral field spectroscopic mapping of the Wolf-Rayet planetary nebula Th 2-A, obtained using the Wide Field Spectrograph on the Australian National University 2.3-m telescope.…

Solar and Stellar Astrophysics · Physics 2015-12-09 Ashkbiz Danehkar

We report the detection of spiral substructure in both the gas velocity and temperature structure of the disk around TW~Hya, suggestive of planet-disk interactions with an unseen planet. Perturbations from Keplerian rotation tracing out a…

Earth and Planetary Astrophysics · Physics 2019-11-06 Richard Teague , Jaehan Bae , Jane Huang , Edwin Bergin

We present X-ray spectral analysis of the accreting young star TW Hydrae from a 489 ks observation using the Chandra High Energy Transmission Grating. The spectrum provides a rich set of diagnostics for electron temperature T_e, electron…

Solar and Stellar Astrophysics · Physics 2015-05-14 N. S. Brickhouse , S. R. Cranmer , A. K. Dupree , G. J. M. Luna , S. Wolk

We present interferometric observations with the Atacama Large Millimeter Array (ALMA) of the free-free continuum and recombination line emission at 1 and 3mm of the "Red Square Nebula" surrounding the B[e]-type star MWC922. The unknown…

Solar and Stellar Astrophysics · Physics 2019-09-18 C. Sánchez Contreras , A. Báez-Rubio , J. Alcolea , A. Castro-Carrizo , V. Bujarrabal , J. Martín-Pintado , D. Tafoya

The cTTS TW Hya has been observed with high-resolution X-ray spectrometers. Previously found high densities inferred from He-like f/i triplets strongly suggested the detected X-ray emission to be dominated by an accretion shock. Because of…

Astrophysics · Physics 2009-11-11 Jan-Uwe Ness , Juergen H. M. M. Schmitt

I model profiles of the [NeII] forbidden emission line at 12.81um, emitted by photoevaporative winds from discs around young, solar-mass stars. The predicted line luminosities (~ 1E-6 Lsun) are consistent with recent data, and the line…

Astrophysics · Physics 2009-11-13 R. D. Alexander

We present a detailed comparison of optical H II region spectra to photoionization models based on modern stellar atmosphere models. We examine both spatially resolved and integrated emission-line spectra of the HII regions DEM L323, DEM…

Astrophysics · Physics 2009-09-25 M. S. Oey , M. A. Dopita , J. C. Shields , R. C. Smith

We present the first high angular resolution 1.4mm and 2.7mm continuum maps of the T Tauri binary system HK Tau obtained with the Plateau de Bure Interferometer. The contributions of both components are well disentangled at 1.4mm and the…

Astrophysics · Physics 2009-11-07 G. Duchene , F. Menard , K. Stapelfeldt , G. Duvert

We present high resolution (R = 100,000) L-band spectroscopy of 11 Herbig AeBe stars with circumstellar disks. The observations were obtained with the VLT/CRIRES to detect hot water and hydroxyl radical emission lines previously detected in…

Solar and Stellar Astrophysics · Physics 2015-05-27 D. Fedele , I. Pascucci , S. Brittain , I. Kamp , P. Woitke , J. P. Williams , W. R. F. Dent , W. -F. Thi

We present high-resolution imaging of the young binary T Tauri in 3 mm continuum emission. Compact dust emission with integrated flux density 50 +/- 6 mJy is resolved in an aperture synthesis map at 0.5" resolution and is centered at the…

Astrophysics · Physics 2009-10-30 R. L. Akeson , D. W. Koerner , E. L. N. Jensen