J/A+A/446/485        New very low-mass members in Taurus         (Guieu+, 2006)

Seventeen new very low-mass members in Taurus. The brown dwarf deficit revisited. Guieu S., Dougados C , Monin J-L , Magnier E., Martin E.L <Astron. Astrophys. 446, 485 (2006)> =2006A&A...446..485G 2006A&A...446..485G
ADC_Keywords: Stars, M-type ; Stars, dwarfs ; Photometry, infrared Keywords: stars: low-mass, brown dwarfs - stars: late-type - stars: luminosity function, mass function - stars: pre-main sequence Abstract: We have performed a large scale optical survey of the Taurus cloud, covering a total area of 28deg2, and encompassing the densest parts of the cloud as well as their surroundings, down to a mass detection limit of 15 Jupiter masses. We present the optical spectroscopic follow-up observations of 97 photometrically selected potential new low-mass Taurus members, of which 27 are strong late-M spectral type SpType<M4V candidates. We derive spectral types, visual absorption and luminosity class estimates and discuss our criteria to assess Taurus membership. These observations reveal 5 new VLM Taurus members and 12 new brown dwarfs. Combining our observations with previously published results, we derive an updated substellar to stellar ratio in Taurus of Rss=0.23±0.05. This ratio now appears consistent with the value previously derived in the Trapezium cluster under similar assumptions of 0.26±0.04. We find indications that the relative numbers of brown dwarfs with respect to stars is decreased by a factor 2 in the central regions of the aggregates with respect to the more distributed population. Our findings are best explained in the context of the embryo-ejection model where brown dwarfs originate from dynamical interactions in small N unstable multiple systems. Description: Derived parameters and spectral properties of sources identified as field stars or with uncertain membership (table 3) and for confirmed Taurus members (table 4). Table 5 present photometry and derived parameters for previous known (top) and new (bottom) Taurus Brown Dwarfs and very low mass stars File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table3.dat 90 74 Derived parameters and spectral properties of sources identified as field stars or with uncertain membership table4.dat 90 23 Same as table 3 for confirmed Taurus members table5.dat 62 23 Photometry and derived parameters for previously known and new Taurus BD and VLM members -------------------------------------------------------------------------------- See also: J/AJ/127/2856 : Brown dwarfs in the 2MASS Survey (Burgasser+, 2004) Byte-by-byte Description of file: table3.dat table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 17 A17 ---- 2MASS 2MASS Name 18 A1 ---- n_2MASS [*] *: candidates not selected with the primary selection method (see Sect. 2.1) 20- 31 A12 ---- Name Target Name (only in table4.dat) 33 I1 ---- Run Run identification number 35- 36 I2 h RAh Right ascension (J2000) 38- 39 I2 min RAm Right ascension (J2000) 41- 46 F6.3 s RAs Right ascension (J2000) 48 A1 --- DE- Declination sign (J2000) 49- 50 I2 deg DEd Declination (J2000) 52- 53 I2 arcmin DEm Declination (J2000) 55- 60 F6.3 arcsec DEs Declination (J2000) 62- 66 F5.2 mag AV Extinction in V band 68- 72 F5.2 0.1nm EWNa Equivalent width of Na line 74- 80 F7.2 0.1nm EWHa Equivalent width of Halpha line 82- 86 A5 --- SpType MK spectral type (Mn.nn) 88- 90 A3 --- LClass Luminosity class derived from spectral fitting -------------------------------------------------------------------------------- Byte-by-byte Description of file: table5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 A12 ---- Name Target Name 14- 18 A5 ---- SpType MK spectral type 20- 22 F3.1 mag AV Extinction in V band 24- 30 F7.4 [solLum] log10(L) logarithm of luminosity 32- 35 I4 K Teff Effective Temperature 37- 41 F5.2 mag Imag I magnitude 43- 46 F4.2 mag I-z ?=- I-z color index 48- 51 F4.2 mag J-H J-H color index 53- 56 F4.2 mag H-Ks H-K color index 58- 62 F5.2 mag Ksmag Ks magnitude -------------------------------------------------------------------------------- Acknowledgements: Sylvain Guieu, sylvain.guieu(at)obs.ujf-grenoble.fr
(End) Sylvain Guieu [LAG], Patricia Vannier [CDS] 04-Oct-2005
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