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    31. Young stellar clusters in the star forming region NGC 6357
    ... The dot-dashed line marks the locus of Classical T-Tauri Stars. Clearly, most of the pre-main sequence stars in the V vs. ... between the 1 and 10 Myr isochrones) are X-ray emitters and spread parallel to the classical T-Tauri locus in the J - H vs ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/precedenti/204-scientific-news/802-ngc6357 -- 44.1 Кб -- 10.04.2016
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    32. http://www.arcetri.astro.it/~fmassi/projects/eng.curr.pdf
    ... Astronomy & Astrophysics 543, A65 (2012) · Vural J., et al. (including Massi F.): "Revealing the inner circumstellar disk of the T Tauri star S Coronae Australis N using the VLTI" Astronomy & Astrophysics 543, A162 (2012) · Wang Y., et al. (including ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~fmassi/projects/eng.curr.pdf -- 112.1 Кб -- 02.12.2015
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    33. http://www.arcetri.astro.it/~fmassi/projects/curr.pdf
    ... Astronomy & Astrophysics 543, A65 (2012) · Vural J., et al. (incluso Massi F.): "Revealing the inner circumstellar disk of the T Tauri star S Coronae Australis N using the VLTI" Astronomy & Astrophysics 543, A162 (2012) · Wang Y., et al. (incluso Massi F ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~fmassi/projects/curr.pdf -- 135.7 Кб -- 02.12.2015
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    34. http://www.arcetri.astro.it/~lt/projects/kona.ps.gz
    ... If BDs form from core 1 2 Testi et al. collapse, they should be associated to disks similar in properties to those found around low mass pre-main{sequence stars (T Tauri stars; TTS). ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~lt/projects/kona.ps.gz -- 37.4 Кб -- 11.09.2007
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    35. http://www.arcetri.astro.it/~lt/preprints/bd40_fig_aa/bd40_fig_aa.ps.gz
    ... Unlike these objects, the colors of the ma­ jority of classical T Tauri stars are more similar to those of heavily reddened main­sequence stars and can be ac­ counted for by standard disk models (e.g. Adams et al. ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/bd40_fig_aa/bd40_fig_aa.ps.gz -- 278.7 Кб -- 11.09.2007
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    36. http://www.arcetri.astro.it/~lt/preprints/hae_dust/natta.ps.gz
    ... The spectral energy distribution (SED) of T Tauri stars at millimeter and submillimeter wavelengths has a shallow dependence on wavelength, consistent with opti- cally thin emission from millimeter-size grains (Beckwith & Sargent 1991). ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/hae_dust/natta.ps.gz -- 92.9 Кб -- 11.09.2007
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    37. http://www.arcetri.astro.it/~lt/preprints/herbig/herbig.ps.gz
    ... A problem in using this method to discriminate be­ tween young stars (members of the cluster) and field stars, is that some kind of young stars (the Weak Line T­Tauri stars or in general the infrared Class III sources) do not show infrared excess at all. ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/herbig/herbig.ps.gz -- 262.6 Кб -- 11.09.2007
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    38. http://www.arcetri.astro.it/~lt/projects/ele_lav.pdf
    ... A.I., Ray T.P., EislЁ el J., 2002, "The kinematic relationship between disk off and jet in the DG Tauri system", A&A, 394, L31 ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~lt/projects/ele_lav.pdf -- 155.2 Кб -- 29.03.2011
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    39. http://www.arcetri.astro.it/~francio/papers/cs14_flames.pdf
    ... We also identified Classical T Tauri Stars (CTTSs) in the two clusters and measured their mass accretion rates. ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~francio/papers/cs14_flames.pdf -- 1945.4 Кб -- 16.11.2006
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    40. HAEBE Clusters Analysis (Abstract)
    ... The stellar volume densities estimated for the groups surrounding pre-main-sequence stars of intermediate mass show the transition from the low density aggregates of T Tauri stars and the dense clusters around massive stars. ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/haebe3/abstract.html -- 2.9 Кб -- 11.09.2007
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