NEW EXTINCTION AND MASS ESTIMATES FROM OPTICAL PHOTOMETRY OF THE VERY LOW MASS BROWN DWARF COMPANION CT CHAMAELEONTIS B WITH THE MAGELLAN AO SYSTEM

被引:17
作者
Wu, Ya-Lin [1 ]
Close, Laird M. [1 ]
Males, Jared R. [1 ]
Barman, Travis S. [2 ]
Morzinski, Katie M. [1 ]
Follette, Katherine B. [1 ]
Bailey, Vanessa [1 ]
Rodigas, Timothy J. [1 ,3 ]
Hinz, Philip [1 ]
Puglisi, Alfio [4 ]
Xompero, Marco [4 ]
Briguglio, Runa [4 ]
机构
[1] Univ Arizona, Steward Observ, Tucson, AZ 85721 USA
[2] Univ Arizona, Lunar & Planetary Lab, Tucson, AZ 85721 USA
[3] Carnegie Inst Sci, Dept Terr Magnetism, Washington, DC 20015 USA
[4] Osserv Astrofis Arcetri, INAF, I-50125 Florence, Italy
基金
美国国家科学基金会;
关键词
brown dwarfs; instrumentation: adaptive optics; planetary systems; planets and satellites: individual (CT Cha B); stars: individual (CT Cha); stars: pre-main sequence; CHAMELEON-I; STELLAR POPULATION; STARS; SPECTRA; EMISSION; CENSUS;
D O I
10.1088/0004-637X/801/1/4
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We used the Magellan adaptive optics system and its VisAO CCD camera to image the young low mass brown dwarf companion CT Chamaeleontis B for the first time at visible wavelengths. We detect it at r', i', z', and Y-S. With our new photometry and T-eff similar to 2500 K derived from the shape of its K-band spectrum, we find that CT Cha B has A(V) = 3.4 +/- 1.1 mag, and a mass of 14-24 M-J according to the DUSTY evolutionary tracks and its 1-5 Myr age. The overluminosity of our r' detection indicates that the companion has significant H alpha emission and a mass accretion rate similar to 6 x 10(-10) M-circle dot yr(-1), similar to some substellar companions. Proper motion analysis shows that another point source within 2 '' of CT Cha A is not physical. This paper demonstrates how visible wavelength adaptive optics photometry (r', i', z', Y-S) allows for a better estimate of extinction, luminosity, and mass accretion rate of young substellar companions.
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页数:6
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