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Nube de Lupus (sección Población de estrellas T Tauri)J. M.; Neuhauser, R.; Terranegra, L. (giugno de 1997). «New "weak-line"--T Tauri stars in Lupus». Astronomy and Astrophysics Supplement series 123: 329-352…38 kB (5041 palabras) - 12:17 24 ene 2024
doi:10.1063/1.3215910. Cieza, L (2007). «The spitzer c2d survey of weak-line T Tauri stars. II New constraints on the timescale for planet building». The…20 kB (2732 palabras) - 04:25 9 oct 2023
Resultados de la Wikipedia en inglés.
- Classical T Tauri star (CTTS) Weak-line T Tauri star (WTTS) Naked T Tauri star (NTTS), which is a subset of WTTS. Roughly half of T Tauri stars have circumstellar…9 kB (928 palabras) - 20:03 20 mar 2024
- III stars have lost their disks and correspond approximately to weak-line T Tauri stars. An intermediate stage where disks can only be detected at longer…5 kB (612 palabras) - 15:29 12 abr 2024
- Herbig–Haro object (sección Source stars)T Tauri stars), but they are still surrounded by disks of dust and gas, and produce weak outflows of low luminosity. Class III objects (Weak-line T Tauri…37 kB (4063 palabras) - 11:44 9 mar 2024
- PDS 70 (categoría T Tauri stars)Herwats, E.; Surdej, J. (2006). "Coronagraphic imaging of three weak-line T Tauri stars: evidence of planetary formation around PDS 70" (PDF). Astronomy…26 kB (2356 palabras) - 05:19 6 abr 2024
- S2CID 16660243. Cieza, L; et al. (2007). "The spitzer c2d survey of weak-line T Tauri stars. II New constraints on the timescale for planet building". The…24 kB (2959 palabras) - 02:11 14 mar 2024
- comparison, the Sun's surface temperature is 5,772 K. V830 Tauri is a weak-lined T Tauri star, a pre-main sequence star that has a surrounding disc producing…10 kB (878 palabras) - 13:43 25 dic 2023
- Aldebaran (redirección desde Alpha Tauri)constellation of Taurus. It has the Bayer designation α Tauri, which is Latinized to Alpha Tauri and abbreviated Alpha Tau or α Tau. Aldebaran varies in…53 kB (5084 palabras) - 19:15 3 may 2024
- Accretion (astrophysics) (sección Accretion of stars)Classical T Tauri stars evolve into weakly lined T Tauri stars. This happens after about 1 million years. The mass of the disk around a classical T Tauri star…39 kB (4340 palabras) - 00:16 28 abr 2024
- V1298 Tauri is a young (23±4 Myr) weakly-lined T Tauri star that is part of the Taurus-Auriga association in the Taurus Molecular Cloud. Alternatively…12 kB (1134 palabras) - 16:51 4 mar 2024
- circumstellar disc of dense gas and dust surrounding a young newly formed star, a T Tauri star, or Herbig Ae/Be star. The protoplanetary disk may also be considered…21 kB (2123 palabras) - 14:34 18 feb 2024
- former do not possess accretion disks. Classical T Tauri stars evolve into weakly lined T Tauri stars. The planetesimals near the outer edge of the terrestrial…75 kB (9132 palabras) - 21:19 18 mar 2024
- Detection of a Superhot 100 Million K X-Ray Flare on the Weak-Lined T Tauri Star V773 Tauri", The Astrophysical Journal, 503 (2): 894–901, Bibcode:1998ApJ…16 kB (1090 palabras) - 17:41 3 dic 2023
- T Chamaeleontis (T Cha), also known as HIP 58285, is a T Tauri star located in the southern circumpolar constellation Chamaeleon. It has an apparent magnitude…16 kB (1274 palabras) - 13:59 9 ene 2024
- Hayashi track (redirección desde Hayashi track stars)much lower ages for solar-type stars in NGC2264 and predicted that these stars were rapidly contracting T Tauri stars. In 1962, Hayashi published a 183-page…24 kB (3733 palabras) - 22:39 23 nov 2023
- Chemically peculiar star (redirección desde He-weak star)peculiarities that set them apart from other stars on or near the main sequence. The Am stars (CP1 stars) show weak lines of singly ionized Ca and/or Sc, but…11 kB (1331 palabras) - 06:32 27 ene 2024
- PDS 110 (categoría Pre-main-sequence stars)(2008). "Towards the main sequence: Detailed analysis of weak line and post-T Tauri stars". Monthly Notices of the Royal Astronomical Society. 387 (3):…6 kB (423 palabras) - 04:01 20 dic 2022
- Herbig Ae/Be star (redirección desde Herbig AeBe stars)distinguished them from other stars in 1960. The original Herbig criteria were: Spectral type earlier than F0 (in order to exclude T Tauri stars), Balmer emission…5 kB (567 palabras) - 21:27 12 sep 2022
- Mercury-manganese star (redirección desde HgMn stars)peculiar star with a prominent spectral line at 398.4 nm, due to absorption from ionized mercury. These stars are of spectral type B8, B9, or A0, corresponding…4 kB (315 palabras) - 23:54 2 may 2024
- Wolf–Rayet star (redirección desde Wolf-Rayet stars)hydrogen lines usually weak or absent. Initially simply referred to as class W or W-type stars, the classification was then split into stars with dominant lines…96 kB (10 597 palabras) - 16:01 2 may 2024
- invoked by Bastien, Robert and Nadeau, to explain the CP measured in 6 T-Tauri stars at a wavelength of 768 nm. They found a maximum CP of q ∼ 7 × 10 − 4…14 kB (1695 palabras) - 16:59 24 feb 2024
- luminosity, and levels of lithium may indicate that this is instead a weak-lined T Tauri star—a low mass pre-main sequence star that is relatively poor in…5 kB (358 palabras) - 10:29 26 nov 2022