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

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Wide field near-infrared observations and Spitzer Space Telescope IRAC observations of the DR21/W75 star formation regions are presented. The photometric data are used to analyse the extinction, stellar content and clustering in the entire…

天体物理学 · 物理学 2008-11-26 M. S. N. Kumar , C. J. Davis , J. M. C. Grave , B. Ferreira , D. Froebrich

We present basic atmospheric parameters (Teff, logg, vt and [Fe/H]) as well as luminosities, masses, radii and absolute radial velocities for 348 stars, presumably giants, from the ~1000 star sample observed within the Penn State-Torun…

地球与行星天体物理 · 物理学 2015-06-05 P. Zielinski , A. Niedzielski , A. Wolszczan , M. Adamow , G. Nowak

We have carried out a deep near-infrared survey of a bright-rimmed molecular cloud, BRC 14 (IC 1848A). The 10 sigma limiting magnitude of the survey is 17.7 mag at the K-band. Seventy-four sources are classified as young stellar object…

天体物理学 · 物理学 2015-06-24 Ikuko Matsuyanagi , Yoichi Itoh , Koji Sugitani , Yumiko Oasa , Tadashi Mukai , Motohide Tamura

The southern Galactic high mass star-forming region, G351.6-1.3, is a HII region-molecular cloud complex with a luminosity of 2.0 x 10^5 L_sun, located at a distance of 2.4 kpc. In this paper, we focus on the investigation of the associated…

星系天体物理 · 物理学 2015-06-19 S. Vig , S. K. Ghosh , D. K. Ojha , R. P. Verma , M. Tamura

We present new nearby stars extracted from a proper motion catalogue and having a DENIS counterpart. Their distances and spectral type are estimated using the DENIS colours. 107 stars are within 50 pc. 31 stars among them have previously…

天体物理学 · 物理学 2009-11-07 C. Reyle , A. C. Robin , R. -D. Scholz , M. Irwin

We obtained deep near-infrared images of Sh 2-208, one of the lowest-metallicity HII regions in the Galaxy, [O/H] = -0.8 dex. We detected a young cluster in the center of the HII region with a limiting magnitude of K = 18.0 mag (10sigma),…

星系天体物理 · 物理学 2016-04-27 Chikako Yasui , Naoto Kobayashi , Masao Saito , Natsuko Izumi

We present optical and near-IR spectroscopy (600--1000 nm) of 8 faint (I$>$18) very red (R--I$>$2.2) objects discovered in a deep CCD survey of the Pleiades (Zapatero-Osorio et al. 1996). We compare them with reliable cluster members like…

天体物理学 · 物理学 2010-04-21 E. L. Martin , R. Rebolo , M. R. Zapatero Osorio

We present results of an optical and near-infrared (IR) 1.8 deg^2 survey in the Pleiades open cluster to search for substellar objects. From optical I-band images from the CFHT and J-band images from the 3.5 m CAHA Telescope, we identify 18…

天体物理学 · 物理学 2009-11-11 G. Bihain , R. Rebolo , V. J. S. Bejar , J. A. Caballero , C. A. L. Bailer-Jones , R. Mundt

We presented 15 new T dwarfs that were selected from UKIRT Infrared Deep Sky Survey, Visible and Infrared Survey Telescope for Astronomy, and Wide-field Infrared Survey Explorer surveys, and confirmed with optical to near infrared spectra…

太阳与恒星天体物理 · 物理学 2019-05-01 Z. H. Zhang , A. J. Burgasser , M. C. Galvez-Ortiz , N. Lodieu , M. R. Zapatero Osorio , D. J. Pinfield , F. Allard

Briceno et al. recently used optical imaging, data from the Two-Micron All-Sky Survey (2MASS), and follow-up spectroscopy to search for young low-mass stars and brown dwarfs in 8 square degrees of the Taurus star-forming region. By the end…

The results of a search for cool subdwarfs are presented. Kinematic (U, V, and W) and stellar parameters (Teff, log g, [Fe/H], and V_t) are derived for 134 candidate subdwarfs based on high resolution spectra. The observed stars span 4200K…

天体物理学 · 物理学 2009-11-07 David Yong , David L. Lambert

We present a distant T$-$type brown dwarf candidate at $\approx2.55$ kpc discovered in the Cosmic Evolution Early Release Science (CEERS) fields by James Webb Space Telescope (JWST) NIRCam. In addition to the superb sensitivity, we utilised…

Super-luminous supernovae of type Ic have a tendency to occur in faint host galaxies which are likely to have low mass and low metallicity. PTF12dam is one of the closest and best studied super-luminous explosions that has a broad and…

The extent to which star formation varies in galaxies with low masses, low metallicities, and high star formation rate surface densities is not well-constrained. To gain insight into star formation under these physical conditions, this…

星系天体物理 · 物理学 2015-06-18 Amanda A. Kepley , Amy E. Reines , Kelsey E. Johnson , Lisa May Walker

We present the results of a deep (J ~ 21 mag at 5 sigma) infrared photometric survey of a 0.95 square degree area in the central region of the Upper Sco association. The photometric observations consist of a deep (Y+J)-band images obtained…

太阳与恒星天体物理 · 物理学 2015-05-30 N. Lodieu , N. C. Hambly , P. D. Dobbie , N. J. G. Cross , L. Christensen , E. L. Martin , L. Valdivielso

We present sub-arcsec (FWHM ~ 0.5") J, H, K and L' images of a young stellar cluster associated with a candidate massive protostar IRAS22134+5834. The observations reveal a centrally symmetric, flattened cluster enclosing a central dark…

天体物理学 · 物理学 2009-11-10 M. S. Nanda Kumar , D. K. Ojha , C. J. Davis

This paper presents a sensitive and comprehensive IRAC 3-8 $\mu$m photometric survey of white dwarfs for companions in the planetary mass regime with temperatures cooler than the known T dwarfs. The search focuses on descendents of…

天体物理学 · 物理学 2009-11-13 J. Farihi , E. E. Becklin , B. Zuckerman

We present a 1.3 mm continuum survey of the young (2-3 Myr) stellar cluster IC 348, which lies at a distance of 310 pc, and is dominated by low-mass stars (M$_{\star}$ $\sim$ 0.1-0.6 M$_{\odot}$). We observed 136 Class II sources (disks…

The young stellar cluster illuminating the W40 H II region, one of the nearest massive star forming regions, has been observed with the ACIS detector on board the Chandra X-ray Observatory. Due to its high obscuration, this is a…

太阳与恒星天体物理 · 物理学 2015-05-20 Michael A. Kuhn , Konstantin V. Getman , Eric D. Feigelson , Bo Reipurth , Steven A. Rodney , Gordon P. Garmire

We report on the properties of pre-main-sequence objects in the Taurus molecular clouds as observed in 7 mid- and far-infrared bands with the Spitzer Space Telescope. There are 215 previously-identified members of the Taurus star-forming…