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Related papers: Spitzer observations of a 24 micron shadow: Bok Gl…

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We trace the peripheral magnetic field structure of Bok globule CB130, by estimating the linear polarization of its field stars in the R band. The magnetic field orientation sampled by these stars, aligned on average among themselves and…

Solar and Stellar Astrophysics · Physics 2016-09-07 A. Chakraborty , H. S. Das

We present high angular resolution SMA and Spitzer observations toward the Bok globule CB17. SMA 1.3mm dust continuum images reveal within CB17 two sources with an angular separation of about 21" (about 5250 AU at a distance of 250 pc). The…

Solar and Stellar Astrophysics · Physics 2015-06-04 Xuepeng Chen , Hector G. Arce , Michael M. Dunham , Qizhou Zhang , Tyler L. Bourke , Ralf Launhardt , Markus Schmalzl , Thomas Henning

We present a near-infrared extinction study of the dark globule B335, a protostellar collapse candidate, using data from HST/NICMOS and the W.M. Keck Observatory. These data allow a new quantitative test of the "inside-out" collapse model…

In this paper, the results obtained from the polarimetric study of a Bok globule CB17 in both optical and sub-millimeter wavelength are presented. The optical polarimetric observations in R-band ($\lambda$ = 630 nm, $\Delta \lambda$ = 120…

Solar and Stellar Astrophysics · Physics 2019-06-05 G. B. Choudhury , A. Barman , H. S. Das , B. J. Medhi

We study the polarization efficiency (defined as the ratio of polarization to extinction) of stars in the background of the small, nearly spherical and isolated Bok globule CB4 to understand the grain alignment process. A decrease in…

Solar and Stellar Astrophysics · Physics 2015-06-17 Ajoy Barman , Himadri Sekhar Das

Distances to Bok globules and small dark nebulae are important for a variety of reasons. We provide new distance estimates to several small clouds, some of them known to harbor YSO and molecular outflows, and thus being of particular…

Astrophysics of Galaxies · Physics 2010-03-15 Jens Knude , Nadia Kaltcheva

We present Herschel observations of the isolated, low-mass star-forming Bok globule CB244. It contains two cold sources, a low-mass Class 0 protostar and a starless core, which is likely to be prestellar in nature, separated by 90 arcsec (~…

Solar and Stellar Astrophysics · Physics 2015-05-18 A. Stutz , R. Launhardt , H. Linz , O. Krause , T. Henning , J. Kainulainen , M. Nielbock , J. Steinacker , P. Andre

We present Spitzer observations of a sample of 12 starless cores selected to have prominent 24 micron shadows. The Spitzer images show 8 and 24 micron shadows and in some cases 70 micron shadows; these spatially resolved absorption features…

We used near-infrared 2MASS data to construct visual extinction maps of a sample of Southern Bok globules utilizing the NICE method. We derived radial extinction profiles of dense cores identified in the globules and analyzed their…

Astrophysics · Physics 2009-09-28 Germán A. Racca , José W. S. Vilas-Boas , Ramiro de la Reza

We present infrared and millimeter observations of Barnard 335, the prototypical isolated Bok globule with an embedded protostar. Using Spitzer data we measure the source luminosity accurately; we also constrain the density profile of the…

On the basis of near-infrared imaging observations, we derived visual extinction (Av) distribution toward ten Bok globules through measurements of both the color excess (E_{H-K}) and the stellar density at J, H, and Ks (star count). Radial…

We present a near-infrared extinction study of the dark globule L694-2, a starless core that shows strong evidence for inward motions in molecular line profiles. The J,H, and K band data were taken using the European Southern Observatory…

We present Spitzer observations of IC 443 obtained with MIPS and IRS as part of our GTO program on the astrophysics of ejecta from evolved stars. We find that the overall morphology at mid/far IR wavelengths resembles even more closely a…

Astrophysics · Physics 2008-04-30 A. Noriega-Crespo , D. C. Hines , K. Gordon , F. R. Marleau , G. H. Rieke , J. Rho , W. B. Latter

We describe a near-infrared imaging survey of Globule 2 in the Coalsack. This Bok globule is the highest density region of this southern hemisphere molecular cloud and is the most likely location for young stars in this complex. The survey…

Astrophysics · Physics 2009-11-07 German Racca , Mercedes Gomez , Scott J. Kenyon

We present sub-arcsecond resolution millimeter-wave images of a circumstellar disk in the Bok globule CB26. The presence of an edge-on disk is confirmed by the dust continuum morphology and the velocity field of 13CO emission, which…

Astrophysics · Physics 2009-11-07 R. Launhardt , A. I. Sargent

We present the observation of a secondary eclipse of the young hot Neptune, AU Mic b, in the infrared using the Spitzer Space Telescope. Using a primary transit from Spitzer to constrain the system parameters, we tentatively detect an…

We report measurements of the thermal emission of the young and massive planet CoRoT-2b at 4.5 and 8 microns with the Spitzer Infrared Array Camera (IRAC). Our measured occultation depths are 0.510 +- 0.042 % and 0.41 +- 0.11 % at 4.5 and 8…

Observations of the circumstellar disk in the Bok globule CB 26 at 110, 230, and 270 GHz are presented together with the results of the simulations and estimates of the disk parameters. These observations were obtained using the SMA, IRAM…

Solar and Stellar Astrophysics · Physics 2013-02-19 V. Akimkin , Ya. Pavlyuchenkov , R. Launhardt , T. Bourke

We present 12CO (J=2-1) sensitive molecular line and 1.3 mm continuum observations made with the Submillimeter Array (SMA) of the bipolar outflow associated with the young star located in the Bok globule known as CB 26. The SMA observations…

Solar and Stellar Astrophysics · Physics 2023-03-01 J. A. López-Vázquez , Luis A. Zapata , Chin-Fei Lee

Photometric observations in the R and I bands of the detached M-type double-lined eclipsing binary CU Cnc have been acquired and analysed. The photometric elements obtained from the analysis of the light curves have been combined with an…

Astrophysics · Physics 2009-11-07 I. Ribas
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