Identifying nearby, Young, Late-type Stars by Means of their Circumstellar Disks
Abstract
It has recently been shown that a significant fraction of late-type members of nearby, very young associations (age lsim10 Myr) display excess emission at mid-IR wavelengths indicative of dusty circumstellar disks. We demonstrate that the detection of mid-IR excess emission can be utilized to identify new nearby, young, late-type stars including two definite new members ("TWA 33" and "TWA 34") of the TW Hydrae Association (TWA). Both new TWA members display mid-IR excess emission in the Wide-field Infrared Survey Explorer catalog and they show proper motion and youthful spectroscopic characteristics—namely, Hα emission, strong lithium absorption, and low surface gravity features consistent with known TWA members. We also detect mid-IR excess—the first unambiguous evidence of a dusty circumstellar disk—around a previously identified UV-bright, young, accreting star (2M1337) that is a likely member of the Lower-Centaurus Crux region of the Scorpius-Centaurus Complex.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- October 2012
- DOI:
- 10.1088/0004-637X/757/2/163
- arXiv:
- arXiv:1208.4517
- Bibcode:
- 2012ApJ...757..163S
- Keywords:
-
- brown dwarfs;
- circumstellar matter;
- open clusters and associations: individual: TW Hydrae Association;
- stars: evolution;
- stars: low-mass;
- stars: pre-main sequence;
- Astrophysics - Solar and Stellar Astrophysics
- E-Print:
- ApJ, Accepted