Transition disk stars in the NGC 2264 cluster - Accretion diagnostic

In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 48, no. 1

A.p. Sousa - S.h.p. Alencar

Detaily:

Rok, strany: 2018, 302 - 304

Kľúčové slová:

open clusters and associations: individual: NGC 2264, stars: pre-main sequence, accretion, accretion disks

URL originálneho zdroja: http://www.astro.sk/caosp/Eedition/Abstracts/2018/Vol_48/No_1/pp302-304_abstract.html

Full text

O článku:

Disk holes are inferred from infrared observations of T Tauri stars, indicating the existence of a transitional phase between thick accreting disks and debris disks. Using data from the observational multiwavelength campaign CSI2264, we analyzed 410 stars belonging to NGC 2264 and found about 7% transition disk candidates. We characterized these star-disk systems using accretion diagnostics and we compared them with star-disk systems with full disks and diskless. We were able to evaluate the influence of disk evolution on the observed accretion characteristics.

Ako citovať:

ISO 690:

Sousa, A., Alencar, S. 2018. Transition disk stars in the NGC 2264 cluster - Accretion diagnostic. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 48, no.1, pp. 302-304. 1335-1842.

APA:

Sousa, A., Alencar, S. (2018). Transition disk stars in the NGC 2264 cluster - Accretion diagnostic. Contributions of the Astronomical Observatory Skalnaté Pleso, 48(1), 302-304. 1335-1842.