A Flaring L5 Dwarf: The Nature of Hα Emission in Very Low Mass (Sub)Stellar Objects
Abstract
Time series spectrophotometry of the L5 dwarf 2MASS J01443536-0716142 showed strong Hα emission that declined by nearly 75% in four consecutive exposures. The line was not detected in emission on a spectrum obtained 11 months later. This behavior contrasts with that of 2MASSI J1315309-264951, an L5 dwarf that has shown even stronger Hα emission on four separate occasions. The observational database suggests that L dwarfs can be found in such strong flares only occasionally, with a duty cycle on the order of 1%. In contrast, the few, continuously strong Hα emitters, including PC 0025+0447 and 2MASSI J1237392+652615, must either be (1) objects no older than 10-100 Myr with continuously active accretion and/or chromospheres, but which apparently formed in isolation from known young stellar clusters and associations, or (2) objects empowered by a different but unknown mechanism for the Hα energy.
- Publication:
-
The Astronomical Journal
- Pub Date:
- January 2003
- DOI:
- 10.1086/345514
- arXiv:
- arXiv:astro-ph/0210348
- Bibcode:
- 2003AJ....125..343L
- Keywords:
-
- Stars: Chromospheres;
- stars: individual (2MASS J01443536-0716142);
- stars: individual (2MASSI J1315309-264951);
- stars: individual (PC 0025+0447);
- Stars: Individual: Alphanumeric: 2MASSI J1237392+652615;
- Stars: Low-Mass;
- Brown Dwarfs;
- Astrophysics
- E-Print:
- 11 pages, 2 figures, Astronomical Journal in press -- Jan 2003 issue