Physics
Scientific paper
Oct 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994an....315..427s&link_type=abstract
Astronomische Nachrichten (ISSN 0004-6337), vol. 315, no. 6, p. 427-430
Physics
1
Balmer Series, Black Body Radiation, Emission Spectra, Late Stars, Main Sequence Stars, Spectrum Analysis, Stellar Activity, Stellar Physics, T Tauri Stars, Astronomical Catalogs, Boundary Layers, Charge Coupled Devices, Continuum Modeling, Data Reduction, Stellar Mass Accretion, Stellar Spectrophotometry, Stellar Temperature
Scientific paper
We present a flux calibrated spectrum of the star listed as CY Tau in the `General Catalog of Variable Stars 4th ed.' in the spectral range 3700 A less than or equal to lambda less than or equal to 6400 A with a resolution of approximately equals 15 A showing the Balmer-Series from Hbeta to H10 as well as the CaII H (in blend with Hepsilon and K lines in emission. Apart from the emission lines the spectrum is composed of a continuum equivalent to that of an ordinary pre-main sequence star (i.e. a `naked' T Tau) of spectral type M2 V with emission lines plus a `blue' veiling continuum that can be described as black body radiation of temperature TBL approximately equals 7000K due to accretion onto a boundary layer at a rate of M-dotacc greater than or approximately = 2.18 10-8 solar mass/a.
Schultz Reinhard
Stuewe Joachim A.
No associations
LandOfFree
A spectrum of the veiled T Tauri star CY Tau does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with A spectrum of the veiled T Tauri star CY Tau, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A spectrum of the veiled T Tauri star CY Tau will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1069913