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Related papers: Very Low-Mass Objects in the Coronet Cluster: The …

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We present new optical spectroscopy with FLAMES/VLT, near-IR imaging with HAWK-I/VLT, and 870 micron mapping with APEX/LABOCA of the Coronet cluster. The optical data allow to estimate spectral types, extinction and the presence of…

Solar and Stellar Astrophysics · Physics 2015-05-28 Aurora Sicilia-Aguilar , Thomas Henning , Jouni Kainulainen , Veronica Roccatagliata

(Abridged) We have completed the first systematic survey for disks around spectroscopically identified young brown dwarfs and very low mass stars. We have obtained L'-band (3.8 um) imaging for 38 very cool objects in IC 348 and Taurus. Our…

Astrophysics · Physics 2008-11-26 Michael C. Liu , Joan Najita , Alan T. Tokunaga

We present Spitzer 3.6--24 micron photometry and spectroscopy for stars in the 1--3 Myr-old Coronet Cluster, expanding upon the survey of Sicilia-Aguilar et al. (2008). Using sophisticated radiative transfer models, we analyze these new…

Solar and Stellar Astrophysics · Physics 2015-05-27 Thayne Currie , Aurora Sicilia-Aguilar

We report new Spitzer Space Telescope observations from the IRAC and MIPS instruments of the young (~ 3 Myr) sigma Orionis cluster. We identify 336 stars as members of the cluster using optical and near-infrared color magnitude diagrams.…

We report on the analysis of 2MASS near-infrared data of a sample of low-mass stars and brown dwarfs in the sigma Orionis cluster. Youth and cluster membership have been spectroscopically confirmed using the Li I spectral line. We find…

Astrophysics · Physics 2009-11-07 J. M. Oliveira , R. D. Jeffries , M. J. Kenyon , S. A. Thompson , Tim Naylor

We have completed a systematic survey for disks around young brown dwarfs and very low mass stars. By choosing a well-defined sample and by obtaining sensitive thermal IR observations, we can make an unbiased measurement of the disk…

Astrophysics · Physics 2007-05-23 Michael C. Liu , Alan T. Tokunaga , Joan Najita

We present some results from a systematic survey for disks around spectroscopically identified young brown dwarfs and very low mass stars. We find that ~75% of our sample show intrinsic IR excesses, indicative of circum(sub)stellar disks.…

Astrophysics · Physics 2007-05-23 Michael C. Liu

Recent surveys have identified sub-stellar objects down to planetary masses in nearby star-forming regions. Reliable determination of the disk frequency in young brown dwarfs is of paramount importance to understanding their origin. Here we…

Astrophysics · Physics 2016-08-30 Ray Jayawardhana , David R. Ardila , Beate Stelzer , Karl E. Haisch

We present multi-wavelength optical and infrared photometry of 170 previously known low mass stars and brown dwarfs of the 5 Myr Collinder 69 cluster (Lambda Orionis). The new photometry supports cluster membership for most of them, with…

The Coronet Cluster in the nearby R CrA dark cloud offers the rare opportunity to study at least four "class I" protostellar sources as well as one candidate "class 0" source, a Herbig Ae star, and a candidate brown dwarf within a few…

Astrophysics · Physics 2009-11-11 Jan Forbrich , Thomas Preibisch , Karl M. Menten

We present a CCD-based photometric survey covering 870 sq. arcmin in a young stellar cluster around the young multiple star sigma Orionis. Our survey limiting R, I, and Z magnitudes are 23.2, 21.8, and 21.0, respectively. From our…

Astrophysics · Physics 2009-10-31 V. J. S. Bejar , M. R. Zapatero Osorio , R. Rebolo

We present near-infrared long slit and multi-slit spectra of low mass brown dwarf candidates in the Orion Nebula Cluster. The long slit data were observed in the H- & K-bands using NIRI on the Gemini North Telescope. The multi-object…

Astrophysics · Physics 2009-11-13 D. J. Weights , P. W. Lucas , P. F. Roche , D. J. Pinfield , F. Riddick

Age-benchmark brown dwarfs' and planetary-mass objects' spectroscopy is key to characterize substellar evolution. In this paper we present the JHK medium resolution (R~3000) spectra of 25 7-75 M_Jup (spectral types L3.0-M6.0) brown dwarfs…

Solar and Stellar Astrophysics · Physics 2025-08-20 Elena Manjavacas , Mario Gennaro , Sarah Betti , Laurent Pueyo , William Balmer , Massimo Robberto

[abridged] Protoplanetary disks with AU-scale inner clearings, often referred to as transitional disks, provide a unique sample for understanding disk dissipation mechanisms and possible connections to planet formation. Observations of…

Solar and Stellar Astrophysics · Physics 2014-11-20 James Muzerolle , Lori E. Allen , S. Thomas Megeath , Jesus Hernandez , Robert A. Gutermuth

We report on a sensitive infrared search for disks around isolated young planetary-mass objects (PMOs) in the NGC1333 cluster, by stacking 70 Spitzer/IRAC frames at 3.6 and 4.5$\,\mu m$. Our co-added images go >2.3 mag deeper than…

Solar and Stellar Astrophysics · Physics 2023-04-19 Aleks Scholz , Koraljka Muzic , Ray Jayawardhana , Victor Almendros-Abad , Isaac Wilson

We present IRAC/MIPS Spitzer Space Telescope observations of the solar type and the low mass stellar population of the young (~5 Myr) Lambda Orionis cluster. Combining optical and 2MASS photometry, we identify 436 stars as probable members…

Solar and Stellar Astrophysics · Physics 2015-05-19 Jesus Hernandez , Maria Morales-Calderon , Nuria Calvet , L. Hartmann , J. Muzerolle , R. Gutermuth , K. L. Luhman , J. Stauffer

We have performed a census of disks around brown dwarfs in the Sigma Ori cluster using all available images from IRAC onboard the Spitzer Space Telescope. To search for new low-mass cluster members with disks, we have measured photometry…

Astrophysics · Physics 2008-12-18 K. L. Luhman , J. Hernandez , J. J. Downes , L. Hartmann , C. Briceno

We report the results of deep infrared observations of brown dwarf candidates in the Trapezium cluster in Orion. Analysis of the JHK color-color diagram indicates that a large fraction (approx 65% +/- 15%) of the observed sources exhibit…

Astrophysics · Physics 2009-09-15 August Muench , Joao Alves , Charles Lada , Elizabeth Lada

We present new deep UBVRI images and high-resolution multi-object optical spectroscopy of the young (~ 6 - 10 Myr old), relatively nearby (800 pc) open cluster IC 2395. We identify nearly 300 cluster members and use the photometry to…

We present Spitzer IRS mid-infrared (5-35 micron) spectra of a complete flux-limited sample (> 3 mJy at 8 micron) of young stellar object (YSO) candidates selected on the basis of their infrared colors in the Serpens Molecular Cloud.…

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