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Related papers: Evidence for Hco+ Infall toward T Tauri?

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During the early stages of star formation, accretion processes such as infall from the envelope and molecular streamers, and ejection of matter through winds and jets take place simultaneously. The Class 0/I binary [BHB2007] 11 shows…

We report here our latest search for molecular outflows from young brown dwarfs and very low-mass stars in nearby star-forming regions. We have observed three sources in Taurus with the Submillimeter Array and the Combined Array for…

Solar and Stellar Astrophysics · Physics 2015-06-22 Ngoc Phan-Bao , Chin-Fei Lee , Paul T. P. Ho , Cuong Dang-Duc , Di Li

We present a 4.5-4.85 micron R=5000 spectrum of the low mass class I young stellar object GSS 30 IRS1 (L=25L_sun) in the rho Ophiuchus core, observed with the infrared spectrometer (ISAAC) on the Very Large Telescope (VLT-UT1). Strong line…

Astrophysics · Physics 2009-11-07 K. M. Pontoppidan , F. L. Schoeier , E. F. van Dishoeck , E. Dartois

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…

Context. Radio frequency molecular absorption lines appear along sight lines with AV well below 1 mag, revealing the presence of H2 in diffuse gas even when 2.6mm CO emission is absent. Aims. We discuss absorption lines of HCO+, C2H, HCN,…

Astrophysics of Galaxies · Physics 2025-06-17 Harvey Liszt , Maryvonne Gerin

ALMA HCO+ observations of the infrared dark cloud G0.253+0.016 located in the Central Molecular Zone of the Galaxy are presented. The 89 GHz emission is area-filling, optically thick, and sub-thermally excited. Two types of filaments are…

We report the results of a 100 square degree survey of the Taurus Molecular Cloud region in the J = 1-0 transition of 12CO and 13CO. The image of the cloud in each velocity channel includes ~ 3 million Nyquist sampled pixels on a 20" grid.…

Astrophysics · Physics 2009-12-08 Paul F. Goldsmith , Mark Heyer , Gopal Narayanan , Ronald Snell , Di Li , Chris Brunt

Context. Classical T Tauri stars (cTTs) are pre-main sequence stars surrounded by an accretion disk. They host a strong magnetic field, and both magnetospheric accretion and ejection processes develop as the young magnetic star interacts…

Solar and Stellar Astrophysics · Physics 2020-10-14 K. Pouilly , J. Bouvier , E. Alecian , S. H. P. Alencar , A. -M. Cody , J. -F. Donati , K. Grankin , G. A. J. Hussain , L. Rebull , C. P. Folsom

We present OVRO Millimeter Array lambda = 3.4 - 1.2 mm dust continuum and spectral line observations of the accretion disk encircling the T Tauri star LkCa 15. The 1.2 mm dust continuum emission is resolved, and gives a minimum diameter of…

We used the TNG/GIANO instrument to obtain near-IR high-resolution spectra (R~50000) of XZ Tau and DR Tau, two actively accreting T Tauri stars classified as EXors. The analysis of the observed features provides information on the…

Solar and Stellar Astrophysics · Physics 2017-10-11 S. Antoniucci , B. Nisini , K. Biazzo , T. Giannini , D. Lorenzetti , N. Sanna , A. Harutyunyan , L. Origlia , E. Oliva

Ultraviolet spectra from the GHRS instrument on board the Hubble Space Telescope reveal the presence of a mysterious absorption feature in the Mg II h & k lines of the nearby (d=20.0 pc) K5 III star Alpha Tau. The narrow absorption looks…

Astrophysics · Physics 2007-05-23 Brian E. Wood , Graham M. Harper , Hans-Reinhard Mueller , Gary P. Zank

We present the first high-resolution, ground-based observations of HCN and C2H2 toward the T Tauri binary star system GV Tau. We detected strong absorption due to HCN nu_3 and weak C2H2 (nu_3 and nu_2 + (nu_4 + nu_5)^0_+) absorption toward…

Astrophysics · Physics 2009-06-23 E. L. Gibb , K. A. Van Brunt , S. D. Brittain , T. W. Rettig

Most of the observed emission lines and continuum excess from young accreting low mass stars (Classical T Tauri stars -- CTTSs) take place in the star-disk or inner disk region. These regions have a complex emission topology still largely…

Astrophysics · Physics 2009-11-13 L. Podio , P. J. V. Garcia , F. Bacciotti , S. Antoniucci , B. Nisini , C. Dougados , M. Takami

We used the CRIRES spectrograph on the VLT to study the ro-vibrational 12CO/13CO, the Pfund beta and H2 emission between 4.59 and 4.72mu wavelengths toward the BN object, the disk candidate source n, and a proposed dust density enhancement…

Solar and Stellar Astrophysics · Physics 2015-05-14 H. Beuther , H. Linz , A. Bik. , M. Goto , Th. Henning

We present archival high angular resolution ($\sim$ 2$''$) $^{12}$CO(3-2) line and continuum submillimeter observations of the young stellar object HL Tau made with the Submillimeter Array (SMA). The $^{12}$CO(3-2) line observations reveal…

Astrophysics of Galaxies · Physics 2015-06-18 Alba M. Lumbreras , Luis A. Zapata

We are studying the extremely young cluster of M17 to investigate the birth of high-mass stars and the initial mass function. Deep JHKL imaging and K-band spectroscopy from the VLT of 201 stars toward the cluster is presented. The majority…

Astrophysics · Physics 2009-11-11 V. H. Hoffmeister , R. Chini , C. M. Scheyda , D. Nuernberger , N. Vogt , M. Nielbock

Time-domain spectroscopy of the classical accreting T Tauri star, TW Hya, covering a decade and spanning the far UV to the near-infrared spectral regions can identify the radiation sources, the atmospheric structure produced by…

Solar and Stellar Astrophysics · Physics 2015-06-19 A. K. Dupree , N. S. Brickhouse , S. R. Cranmer , P. Berlind , J. Strader , G. H. Smith

We present an analysis of high-resolution spectroscopy of several bright T Tauri stars using the VLT/CRIRES and Keck/NIRSPEC spectrographs, revealing the first detections of emission from HCN and C2H2 in circumstellar disks at near-infrared…

Earth and Planetary Astrophysics · Physics 2015-06-03 A. M. Mandell , J. Bast , E. F. van Dishoeck , G. A. Blake , C. Salyk , M. J. Mumma , G. Villanueva

New subarcsecond FUV observations of T Tau with HST/STIS show spatially resolved structures in the 2"x2" area around the star. The structures show in multiline emission of fluorescent H_2 pumped by Lyman alpha. One emission structure…

Astrophysics · Physics 2009-11-07 José Saucedo , Nuria Calvet , Lee Hartmann , John Raymond

We report spatially resolved spectroscopy of both components of the low-mass pre-main-sequence binary GV Tau. High resolution spectroscopy in the K- and L-bands is used to characterize the stellar properties of the binary and to explore the…

Astrophysics · Physics 2009-11-13 Greg W. Doppmann , Joan R. Najita , John S. Carr