Zobrazeno 1 - 10
of 38
pro vyhledávání: '"Bary, Jeffrey. S."'
Accurate age and mass determinations for young pre-main sequence stars are made challenging by the presence of large-scale starspots. We present results from a near-infrared spectroscopic survey of ten T-Tauri Stars in Taurus-Auriga that characterize
Externí odkaz:
http://arxiv.org/abs/2403.20255
Autor:
Paolino, Facundo Pérez, Bary, Jeffrey S., Petersen, Michael S., Ward-Duong, Kimberly, Tofflemire, Benjamin M., Follette, Katherine B., Mach, Heidi
We present a multi-epoch spectroscopic study of LkCa 4, a heavily spotted non-accreting T Tauri star. Using SpeX at NASA's Infrared Telescope Facility (IRTF), 12 spectra were collected over five consecutive nights, spanning $\approx$ 1.5 stellar rota
Externí odkaz:
http://arxiv.org/abs/2303.01574
Autor:
Beck, Tracy L., Bary, Jeffrey S.
We present results from a survey searching for spatially resolved near-infrared line emission from molecular hydrogen gas in the circumstellar environments of nine young stars: AA Tau, AB Aur, DoAr 21, GG Tau, GM Aur, LkCa 15, LkH$\alpha$ 264, UY Aur
Externí odkaz:
http://arxiv.org/abs/1909.04730
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Bary, Jeffrey S., Petersen, Michael S.
We report the detection of an anomalous accretion flare in the tight eccentric pre-main-sequence binary system DQ Tau. In a multi-epoch survey consisting of randomly acquired low to moderate resolution near-infrared spectra obtained over a period of
Externí odkaz:
http://arxiv.org/abs/1407.3309
Circumbinary Gas Accretion onto a Central Binary: Infrared Molecular Hydrogen Emission from GG Tau A
Autor:
Beck, Tracy L., Bary, Jeffrey. S., Dutrey, Anne, Piétu, Vincent, Guilloteau, Stephane, Lubow, S. H., Simon, M.
We present high spatial resolution maps of ro-vibrational molecular hydrogen emission from the environment of the GG Tau A binary component in the GG Tau quadruple system. The H2 v= 1-0 S(1) emission is spatially resolved and encompasses the inner bi
Externí odkaz:
http://arxiv.org/abs/1205.1526
Variations of the 10 um Silicate Features in the Actively Accreting T Tauri Stars: DG Tau and XZ Tau
Publikováno v:
Astrophys.J.706:L168-L172,2009
Using the Infrared Spectrograph aboard the Spitzer Space Telescope, we observed multiple epochs of 11 actively accreting T Tauri stars in the nearby Taurus-Auriga star forming region. In total, 88 low-resolution mid-infrared spectra were collected ov
Externí odkaz:
http://arxiv.org/abs/0910.3454
Autor:
Bary, Jeffrey S., Matt, Sean P., Skrutskie, Michael F., Wilson, John C., Peterson, Dawn E., Nelson, Matthew J.
We present results from a low resolution (R~300) near-infrared spectroscopic variability survey of actively accreting T Tauri stars (TTS) in the Taurus-Auriga star forming region. Paschen and Brackett series H I recombination lines were detected in 7
Externí odkaz:
http://arxiv.org/abs/0807.1727
Autor:
Bary, Jeffrey S., Weintraub, David A., Shukla, Sonali J., Leisenring, Jarron M., Kastner, Joel H.
We report the discovery of quiescent emission from molecular hydrogen gas located in the circumstellar disks of six pre-main sequence stars, including two weak-line T Tauri stars (TTS), and one Herbig AeBe star, in the Chamaeleon I star forming regio
Externí odkaz:
http://arxiv.org/abs/0801.2765
Publikováno v:
Astrophys.J. 576 (2002) L73-L76
Astronomers have established that for a few million years newborn stars possess disks of orbiting gas and dust. Such disks, which are likely sites of planet formation, appear to disappear once these stars reach ages of 5-10 times 10^6 yr; yet, >= 10^
Externí odkaz:
http://arxiv.org/abs/astro-ph/0207626