Emission line diagnostics for accretion and outflows in young very low-mass stars and brown dwarfs

نویسندگان
چکیده

برای دانلود باید عضویت طلایی داشته باشید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Emission line diagnostics for accretion and outflows in young very low-mass stars and brown dwarfs

We discuss accretion and outflow properties of three very low-mass young stellar objects based on broad-band mid-resolution X-Shooter/VLT spectra. Our targets (FUTauA, 2M1207-39, and Par-Lup3-4) have spectral types between M5 and M8, ages between 1Myr and ∼ 10Myr, and are known to be accreting from previous studies. The final objective of our project is the determination of mass outflow to accr...

متن کامل

Uv Excess Measures of Accretion onto Young Very Low-mass Stars and Brown Dwarfs

Low-resolution spectra from 3000–9000 Å of young low-mass stars and brown dwarfs were obtained with LRIS on Keck I. The excess UV and optical emission arising in the Balmer and Paschen continua yields mass accretion rates ranging from 2×10 to 10 M⊙ yr . These results are compared with HST/STIS spectra of roughly solar-mass accretors with accretion rates that range from 2× 10 to 5 × 10 M⊙ yr . T...

متن کامل

Very Low Mass Stars and Brown Dwarfs in Taurus-Auriga

We present high resolution optical spectra obtained with the HIRES spectrograph on the W. M. Keck I telescope of seven low mass T Tauri stars and brown dwarfs (LMTTs) in Taurus-Auriga. The observed Li I 6708 Å absorption, low surface gravity signatures, and radial velocities confirm that all are members of the Taurus star forming region; no new spectroscopic binaries are identified. Four of the...

متن کامل

Models of very-low-mass stars, brown dwarfs and exoplanets

Within the next few years, GAIA and several instruments aiming to image extrasolar planets will be ready. In parallel, low-mass planets are being sought around red dwarfs, which offer more favourable conditions, for both radial velocity detection and transit studies, than solar-type stars. In this paper, the authors of a model atmosphere code that has allowed the detection of water vapour in th...

متن کامل

Companions of old brown dwarfs , and very low mass stars ⋆

Up to now, most planet search projects have concentrated on F to K stars. In order to considerably widen the view, we have stated a survey for planets of old, nearby brown dwarfs and very low mass stars. Using UVES, we have observed 26 brown dwarfs and very low mass stars. These objects are quite inactive and are thus highly suitable for such a project. Two objects were found to be spectroscopi...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

ژورنال

عنوان ژورنال: EPJ Web of Conferences

سال: 2014

ISSN: 2100-014X

DOI: 10.1051/epjconf/20136408005