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相关论文: Methane T-Dwarf Candidates in the Star Forming Reg…

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We identified 46 unresolved source candidates in the Hubble Ultra Deep Field, down to i775 = 29.5. Unresolved objects were identified using a parameter S, which measures the deviation from the curve-of-growth of a point source. Extensive…

We report our study of two proto-brown dwarf candidates in Taurus, [GKH94]~41 and IRAS~04191+1523B. Based on continuum maps at 102~GHz (or 2.9~mm), spectral types and the spectral energy distribution of both targets, we confirmed the class…

星系天体物理 · 物理学 2017-12-05 C. Dang-Duc , N. Phan-Bao

This study aims to determine the main physical parameters (N(H2) hydrogen column density and Td dust temperature) of the Interstellar medium, and their distribution in the extended star-forming region, which includes IRAS 05156+3643,…

星系天体物理 · 物理学 2021-12-08 E. H. Nikoghosyan , N. M. Azatyan , D. H. Andreasyan , D. S. Baghdasaryan

We have mapped the [C I] emission at 492 GHz toward the supernova remnant Cas A. We detect [C I] emission from the periphery of the diffuse Photon Dominated Region (PDR) covering the disk of Cas A, as traced by the carbon recombination…

天体物理学 · 物理学 2009-11-11 B. Mookerjea , N. G. Kantharia , D. A. Roshi , M. Masur , ;

Interstellar absorption lines up to J"=10 in the (2,0) band and up to J"=6 in the (3,0) band of the C$_2$ $A^1\Pi_u$ - $X^1\Sigma^+_g$ system are detected toward star Cernis 52 (BD+31$^o$ 640) in the Perseus molecular complex. The star lies…

宇宙学与河外天体物理 · 物理学 2015-05-20 Susana Iglesias-Groth

We present new multi-frequency radio continuum imaging of the dwarf starburst galaxy NGC 625 obtained with the Very Large Array. Data at 20, 6, and 3.6 cm reveal global continuum emission dominated by free-free emission, with only mild…

天体物理学 · 物理学 2009-11-10 John M. Cannon , Evan D. Skillman

We present VLT/SINFONI integral field spectroscopy of RCW 34 along with Spitzer/IRAC photometry of the surroundings. RCW 34 consists of three different regions. A large bubble has been detected on the IRAC images in which a cluster of…

We have conducted a search of a 9 deg$^{2}$ region of the CFHTLS around the Milky Way analog M101 (D$\sim$7 Mpc), in order to look for previously unknown low surface brightness galaxies. This search has uncovered 38 new low surface…

星系天体物理 · 物理学 2017-12-06 P. Bennet , D. J. Sand , D. Crnojević , K. Spekkens , D. Zaritsky , A. Karunakaran

Star formation theories are currently divergent regarding the fundamental physical processes that dominate the substellar regime. Observations of nearby young open clusters allow the brown dwarf (BD) population to be characterised down to…

星系天体物理 · 物理学 2015-05-18 C. Alves de Oliveira , E. Moraux , J. Bouvier , H. Bouy , C. Marmo , L. Albert

Stars with very low levels of magnetic activity provide an opportunity for a more quantitative comparison with the Sun during its Maunder minimum. We employ spectra from the RAVE survey in a search for particularly low-activity stars with…

太阳与恒星天体物理 · 物理学 2025-04-29 S. P. Järvinen , K. G. Strassmeier

We present results of optical spectroscopic and BVR_CI_C photometric observations of 77 pre-main sequence (PMS) stars in the Cepheus flare region. A total of 64 of these are newly confirmed PMS stars, originally selected from various…

太阳与恒星天体物理 · 物理学 2014-11-20 M. Kun , Z. Balog , S. J. Kenyon , E. E. Mamajek , R. A. Gutermuth

We present a near infrared study focused on the detection and characterization of the youngest stellar component of the NGC 604 giant star-forming region, in the Triangulum galaxy (M 33). By means of color-color diagrams derived from the…

宇宙学与河外天体物理 · 物理学 2015-06-03 Cecilia Farina , Guillermo L. Bosch , Rodolfo H. Barba

We report trigonometric parallaxes for 134 low mass stars and brown dwarfs, of which 38 have no previously published measurement and 79 more have improved uncertainties. Our survey targeted nearby targets, so 119 are closer than 30 pc. Of…

太阳与恒星天体物理 · 物理学 2016-07-06 A. J. Weinberger , A. P. Boss , S. A. Keiser , G. Anglada-Escudé , I. B. Thompson , G. Burley

T and Y-dwarfs are among the coolest and least luminous objects detected, and they can help to understand the properties of giant planets. Their multiplicity properties can shed light on the formation process. We observed a sample six T…

太阳与恒星天体物理 · 物理学 2015-05-27 N. Huélamo , V. D. Ivanov , R. Kurtev , J. H. Girard , J. Borissova , D. Mawet , K. Muzic , C. Cáceres , C. H. F. Melo , M. F. Sterzik , D. Minniti

We present the current status of PHOENIX model atmospheres for dwarfs of the spectral type T, typical for older field brown dwarfs and low-mass brown dwarfs. The results are based on new predictions of the CH_4 line opacities from…

天体物理学 · 物理学 2007-05-23 D. Homeier , P. H. Hauschildt , F. Allard

We present complete, low resolution IJHK spectroscopy of the ultracompact HII region, G45.12+0.13. From the observed HI line strengths, we derive a near infrared extinction law that is slightly steeper than the average. After correction…

天体物理学 · 物理学 2015-06-24 Stuart Lumsden , Phil Puxley

K-band spectra of young stellar candidates in four southern hemisphere clusters have been obtained with the near-infrared spectrograph GNIRS in Gemini South. The clusters are associated with IRAS sources that have colours characteristic of…

天体物理学 · 物理学 2009-11-13 A. Roman-Lopes , Z. Abraham , R. Ortiz , A. Rodrigues-Ardila

We have performed an optical spectroscopic and photometric search for young stellar objects associated with the molecular cloud Lynds 1340, and examined the structure of the cloud by constructing an extinction map, based on SDSS data. The…

太阳与恒星天体物理 · 物理学 2016-06-09 M. Kun , A. Moór , E. Szegedi-Elek , B. Reipurth

Context. Thanks to recent and ongoing large scale surveys, hundreds of brown dwarfs have been discovered in the last decade. The Canada-France Brown Dwarf Survey is a wide-field survey for cool brown dwarfs conducted with the MegaCam camera…

太阳与恒星天体物理 · 物理学 2015-05-19 C. Reyle , P. Delorme , C. J. Willott , L. Albert , X. Delfosse , T. Forveille , E. Artigau , L. Malo , G. J. Hill , R. Doyon

(Abridged) We report on the near-infrared low-resolution spectroscopy and red optical (Z-band) photometry of seven proper-motion, very low-mass substellar member candidates of the Pleiades cluster with magnitudes in the interval J=17.5-20.8…

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