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Related papers: Two class I very low-mass objects in Taurus

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We observed with the JVLA at 3.6 and 1.3 cm a sample of 11 proto-brown dwarf candidates in Taurus in a search for thermal radio jets driven by the most embedded brown dwarfs. We detected for the first time four thermal radio jets in…

2MASS J03202839-0446358AB is a recently identified, late-type M dwarf/T dwarf spectroscopic binary system for which both the radial velocity orbit for the primary and spectral types for both components have been determined. By combining…

Solar and Stellar Astrophysics · Physics 2009-11-13 Adam J. Burgasser , Cullen H. Blake

With Herschel/PACS 134 low mass members of the Taurus star-forming region spanning the M4-L0 spectral type range and covering the transition from low mass stars to brown dwarfs were observed. Combining the new Herschel results with other…

Solar and Stellar Astrophysics · Physics 2014-10-15 J. Bulger , J. Patience , K. Ward-Duong , C. Pinte , H. Bouy , F. Ménard , J. -L. Monin

We present SCUBA-2 850um observations for 7 very low mass stars (VLMS) and brown dwarfs (BDs): 3 in Taurus, 4 in the TWA, and all classical T Tauri (cTT) analogs. We detect 2 of the 3 Taurus disks, but none of the TWA ones. Our 3sigma…

Measuring the properties of protoplanetary disks around brown dwarfs is central to understanding the formation of brown dwarfs and their planetary companions. We present modeling of CFHT Tau 4 and 2M0444, two brown dwarfs with…

Solar and Stellar Astrophysics · Physics 2019-06-26 Anneliese M. Rilinger , Catherine C. Espaillat , Enrique Macías

We present the results of a search for new members of the Taurus star-forming region using data from the Spitzer Space Telescope and the XMM-Newton Observatory. We have obtained optical and near-infrared spectra of 44 sources that exhibit…

Astrophysics of Galaxies · Physics 2014-11-20 K. L. Luhman , E. E. Mamajek , P. R. Allen , K. L. Cruz

Recent studies of the substellar population in the Taurus cloud have revealed a deficit of brown dwarfs (BD) compared to the Trapezium cluster population (Briceno et al 1998; Luhman 2000; Luhman et al 2003a; Luhman 2004). However, these…

Astrophysics · Physics 2009-11-13 S. Guieu , C Dougados , J. L Monin , E Magnier , E. L Martin

We have performed a survey for substellar companions to young brown dwarfs in the Taurus star-forming region using the Wide Field Planetary Camera 2 on board the Hubble Space Telescope. In these data, we have discovered a candidate…

Astrophysics of Galaxies · Physics 2015-05-18 K. Todorov , K. L. Luhman , K. K. McLeod

We present the results of a deep, optical/IR wide field imaging survey of selected fields in the nearby (d ~ 140 pc) Taurus star-forming region. We report the discovery of 9 new members with spectral types M5.75-M9.5. We derive an Initial…

Astrophysics · Physics 2007-05-23 Cesar Briceno , Kevin Luhman , Lee Hartmann , John Stauffer , Davy Kirkpatrick

Low-mass stars belonging to the M spectral type are the most numerous stars in our Galaxy, amounting to about two-thirds in number, and are found at the bottom of the main sequence in the H-R diagram. %Multi-wavelength studies on…

Solar and Stellar Astrophysics · Physics 2024-01-17 Samrat Ghosh , Soumen Mondal , Santosh Joshi , Sneh Lata , Rajib Kumbhakar

Benchmark brown dwarfs are those objects for which fiducial constraints are available, including effective temperature, parallax, age, metallicity. We searched for new cool brown dwarfs in 186 sq.deg. of the new area covered by the data…

Solar and Stellar Astrophysics · Physics 2015-05-18 B. Goldman , S. Marsat , T. Henning , C. Clemens , J. Greiner

We report the results of a deep near infrared (JHK) survey of the outer parts of the Trapezium Cluster with Gemini South/Flamingos. 396 sources were detected in a 26 arcmin^2 area, including 138 brown dwarf candidates, defined as M<0.075…

Astrophysics · Physics 2009-11-11 P. W. Lucas , P. F. Roche , M. Tamura

We obtained medium-resolution spectra of the bona-fide brown dwarf Cha H$\alpha$ 1, the five brown dwarf candidates Cha H$\alpha$ 2 to 6, two additional late M-type brown dwarf candidates, all originally selected by H$\alpha$ emission, and…

Astrophysics · Physics 2016-08-30 Ralph Neuhaeuser , Fernando Comeron

We present 27 new L subdwarfs and classify five of them as esdL and 22 as sdL. Our L subdwarf candidates were selected with the UKIRT Infrared Deep Sky Survey and Sloan Digital Sky Survey. Spectroscopic follow-up was carried out primarily…

We have used infrared images obtained with the Wide Field Camera 3 on board the Hubble Space Telescope to search for planetary-mass brown dwarfs in the star-forming cluster IC 348. In those images, we have identified 12 objects that have…

Solar and Stellar Astrophysics · Physics 2020-07-22 K. L. Luhman , C. J. Hapich

We report new dynamical masses for 5 pre-main sequence (PMS) stars in the L1495 region of the Taurus star-forming region (SFR) and 6 in the L1688 region of the Ophiuchus SFR. Since these regions have VLBA parallaxes these are absolute…

Solar and Stellar Astrophysics · Physics 2017-08-09 M. Simon , S. Guilloteau , E. di Folco , A. Dutrey , N. Grosso , V. Piétu , E. Chapillon , L. Prato , G. H. Schaefer , E. Rice , Y. Boehler

We report the discovery of an esdL3 subdwarf, ULAS J020858.62+020657.0, and a usdL4.5 subdwarf, ULAS J230711.01+014447.1. They were identified as L subdwarfs by optical spectra obtained with the Gran Telescopio Canarias, and followed up by…

Free-floating planetary mass objects--worlds that roam interstellar space untethered to a parent star--challenge conventional notions of planetary formation and migration, but also of star and brown dwarf formation. We focus on the…

We present the results of a search for new members of the Taurus star-forming region using the Infrared Array Camera (IRAC) aboard the Spitzer Space Telescope}. With IRAC images of 29.7 deg^2 of Taurus at 3.6, 4.5, 5.8, and 8.0 um, we have…

We report here our search for molecular outflows from young very low mass stars and brown dwarfs in Taurus and rho Ophiuchi. Using the Submillimeter Array (SMA) and the Combined Array for Research in Millimeter-wave Astronomy (CARMA), we…

Solar and Stellar Astrophysics · Physics 2015-05-27 Ngoc Phan-Bao , Chin-Fei Lee , Paul T. P. Ho , Ya-Wen Tang