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Related papers: Distance estimation of some selected small Bok glo…

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We have obtained deep near infrared J- and K-band observations of 14 BL Herculis and 5 W Virginis SMC stars from the OGLE III survey with the ESO New Technology Telescope equipped with the SOFI infrared camera. From these observations,…

Astrophysics of Galaxies · Physics 2010-07-27 Ciechanowska A. , Pietrzynski G. , Szewczyk O. , Gieren W. , Soszynski I

We report an accurate distance of d = 10+/-2.5kpc to the high-velocity cloud Complex C. Using high signal-to-noise Keck/HIRES spectra of two horizontal-branch stars, we have detected CaII K absorption lines from the cloud. Significant…

Astrophysics · Physics 2009-11-13 C. Thom , J. E. G. Peek , M. E. Putman , Carl Heiles , K. M. G. Peek , R. Wilhelm

Foreground emission and scattered light from interplanetary dust (IPD) particles and emission from Galactic stellar sources are the greatest obstacles for determining the cosmic infrared background (CIB) from diffuse sky measurements in the…

Astrophysics · Physics 2007-05-23 E. Dwek , R. G. Arendt

We present $BVI$ photometry for about 16000 stars from a 220 arcmin$^{2}$ field centered 8 arcmin east of the center of 47 Tuc. We have identified eight likely blue stragglers located in the outer parts of the cluster. Four of these objects…

Astrophysics · Physics 2007-05-23 J. Kaluzny , A. Wysocka , K. Z. Stanek , W. Krzeminski

Many black hole (BH) candidates exist, ranging from supermassive ($\sim10^{6}$--$10^{10}$ M$_{\odot}$) to stellar masses ($\sim 1$--$100$ M$_{\odot}$), all of them identified by indirect processes. Although there are no known candidate BHs…

Cosmology and Nongalactic Astrophysics · Physics 2014-06-09 J. L. G. Sobrinho , P. Augusto

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 have carried out a morphological search for molecular clouds possibly associated with 48 Galactic infrared bubbles with angular radii of $>1'$ in the southern Galactic plane of $295^\circ \le l\le 350^\circ$ and $|b|\le 1^\circ$…

Astrophysics of Galaxies · Physics 2025-07-03 Mikito Kohno , Yoshiaki Sofue , Yasuo Fukui , Kengo Tachihara

High-precision (sigma < 0.01) new JHK observations of 226 of the brightest and nearest red clump stars in the solar neighbourhood are used to determine distance moduli for the LMC. The resulting K- and H-band values of 18.47\pm0.02 and…

Solar and Stellar Astrophysics · Physics 2015-05-30 C. D. Laney , M. D. Joner , G. Pietrzynski

We present new sub-arcsecond-resolution near-infrared polarimetric imaging and millimetre interferometry data on the circumstellar disk system in the Bok globule CB26. The data imply the presence of a M > 0.01 M_sun edge-on disk of >400 AU…

Astrophysics · Physics 2009-11-06 R. Launhardt , B. Stecklum , A. I. Sargent

A search for variable stars in the globular cluster NGC 288 was carried out using a time-series of CCD images in the $V$ and $I$ filters. The photometry of all stellar sources in the field of view of our images, down to $V\approx19$ mag,…

Solar and Stellar Astrophysics · Physics 2014-01-23 A. Arellano Ferro , D. M. Bramich , S. Giridhar , R. Figuera Jaimes , N. Kains , K. Kuppuswamy

This paper is intended as part of a more extensive molecular line survey in star forming regions along the evolutionary track of a collapsing cloud toward a young stellar object. We have studied a sample of seven small dark clouds (Bok…

Astrophysics · Physics 2009-10-22 F. Scappini , G. G. C. Palumbo , G. Bruni , P. Bergman

We present high angular resolution observations of water masers at 1.3 cm and radio continuum emission at 1.3, 3.6 and 6 cm towards the Bok globule CB 54 using the Very Large Array. At 1.3 cm, with subarsecond angular resolution, we detect…

Astrophysics of Galaxies · Physics 2015-05-13 I. de Gregorio-Monsalvo , J. F. Gomez , G. Anglada , J. M. Torrelles , T. B. H. Kuiper , O. Suarez , N. A. Patel

We present a preliminary report on the first deep infrared photometry of 2MASS GC01 and 2MASS GC02 (GC01 and GC02 hereafter) - new Galactic globular cluster (GC) candidates, discovered by the 2MASS. They both appear to be genuine disk GCs…

Astrophysics · Physics 2007-05-23 Valentin D. Ivanov , Jordanka Borissova , Leonardo Vanzi

We present an analysis of the dust continuum emission at 870 um in order to investigate the mass distribution of clumps within infrared dark clouds (IRDCs). We map six IRDCs with the Large APEX BOlometer CAmera (LABOCA) at APEX, reaching an…

Astrophysics of Galaxies · Physics 2015-06-18 Laura Gomez , Friedrich Wyrowski , Frederic Schuller , Karl Menten , Javier Ballesteros-Paredes

We determine the distances to 18 galaxy clusters with redshifts ranging from z~0.14 to z~0.78 from a maximum likelihood joint analysis of 30 GHz interferometric Sunyaev-Zel'dovich effect (SZE) and X-ray observations. We model the…

Astrophysics · Physics 2010-04-06 E. D. Reese , J. E. Carlstrom , M. Joy , J. J. Mohr , L. Grego , W. L. Holzapfel

InfraRed Dark Clouds (IRDCs) are extinction features against the Galactic infrared background, mainly in mid-infrared band. Recently they were proposed to be potential sites of massive star formation. In this work we have made 12CO, 13CO,…

Astrophysics · Physics 2009-11-13 Fujun Du , Ji Yang

The DIRBE on the COBE spacecraft was designed primarily to conduct systematic search for an isotropic CIB in ten photometric bands from 1.25 to 240 microns. The results of that search are presented here. Conservative limits on the CIB are…

We present a catalog of dust clouds at high Galactic latitude based on the Planck 857 GHz dust emission data. Using a clustering hierarchical algorithm, 315 dust cloud at high Galactic latitudes are identified. Additionally, using the…

Astrophysics of Galaxies · Physics 2024-08-14 Mingxu Sun , Biwei Jiang , Helong Guo , Wenyuan Cui

The high-latitude Galactic H I cloud toward the extragalactic radio source 3C 225 is characterized by very narrow 21 cm emission and absorption indicative of a very low H I spin temperature of about 20 K. Through high-resolution optical…

Astrophysics · Physics 2009-11-11 David M. Meyer , J. T. Lauroesch , Carl Heiles , J. E. G. Peek , Kyle Engelhorn

Based on the largest catalogs currently available, comprising 6090 contact binaries (CBs) and 2167 open clusters, we determine the near-infrared $JHK_{\rm s}$ CB period--luminosity (PL) relations, for the first time achieving the low levels…

Astrophysics of Galaxies · Physics 2016-12-07 Xiaodian Chen , Richard de Grijs , Licai Deng