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Related papers: 2MASS Two-Color Interstellar Reddening Lines in th…

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We observe a sample of 8 evolved stars in the Galactic Bulge in the CO J = 2 - 1 line using the Submillimeter Array (SMA) with angular resolution of 1 - 4 arcseconds. These stars have been detected previously at infrared wavelengths, and…

Solar and Stellar Astrophysics · Physics 2014-08-01 Benjamin A. Sargent , N. A. Patel , M. Meixner , M. Otsuka , D. Riebel , S. Srinivasan

In the course of the NIR/MIR AGN search combining the 6.7 mu ISOCAM Parallel Survey and 2MASS we have discovered 24 type-1 quasars about a third of which are too red to be discriminated by optical/UV search techniques. Here we report on a…

We present {\it UBVI} photometry of the eclipsing binary HV2274 - the system which has been recently used for distance determination to the LMC by Guinan et al. (1998). We determine the interstellar reddening to the star,…

Astrophysics · Physics 2009-10-30 A. Udalski , G. Pietrzynski , P. Wozniak , M. Szymanski , M. Kubiak , K. Zebrun

We measure the extinction law in the 30 Dor star formation region in the Large Magellanic Cloud using Early Release Observations taken with Near-Infrared Camera (NIRCam) onboard the JWST, thereby extending previous studies with the Hubble…

Astrophysics of Galaxies · Physics 2023-03-22 Katja Fahrion , Guido De Marchi

Massive stars are important for the evolution of the interstellar medium. The detailed study of their properties (such as mass loss, rotation, magnetic fields) is enormously facilitated by samples of these objects in young massive galactic…

Astrophysics of Galaxies · Physics 2013-02-08 D. Froebrich

We have pursued two different methods to analyze the old stellar population near the Galactic plane, using data from the 2MASS survey. The first method is based on the isolation of the red clump giant population in the color-magnitude…

Astrophysics · Physics 2009-11-07 M. Lopez-Corredoira , A. Cabrera-Lavers , F. Garzon , P. L. Hammersley

We present measurements of dust reddening using the colors of stars with spectra in the Sloan Digital Sky Survey. We measure reddening as the difference between the measured and predicted colors of a star, as derived from stellar parameters…

Astrophysics of Galaxies · Physics 2011-09-26 Edward F. Schlafly , Douglas P. Finkbeiner

Using infrared photometric data extracted from the 2MASS, IRAS and MSX databases, 142 suspected young stellar objects (YSOs) are selected from about 2 million stars in the Camelopardalis segment of the Milky Way limited by Galactic…

Astrophysics · Physics 2009-06-25 V. Straizys , V. Laugalys

We present infrared (IR) to X-ray spectral energy distributions (SEDs) for 44 red AGN selected from the 2MASS survey on the basis of their red J-K$_S$ color (>2 mag) and later observed by Chandra. In comparison with optically-, radio-, and…

We present a map of the dust reddening to 4.5 kpc derived from Pan-STARRS1 stellar photometry. The map covers almost the entire sky north of declination -30 degrees at a resolution of 7' to 14', and is based on the estimated distances and…

We use near-infrared (J-K)-colours of bright 2MASS galaxies, measured within a 7"-radius aperture, to calibrate the Schlegel et al. (1998) DIRBE/IRAS Galactic extinction map at low Galactic latitudes ($|b| < 10^{\rm o}$). Using 3460…

Astrophysics of Galaxies · Physics 2021-03-10 A. C. Schröder , W. van Driel , R. C. Kraan-Korteweg

Massive clusters in our Galaxy are an ideal testbed to investigate the properties and evolution of high mass stars. They provide statistically significant samples of massive stars of uniform ages. To accurately determine the intrinsic…

Astrophysics of Galaxies · Physics 2015-06-17 Dirk Froebrich , Alexander Scholz

Using the Hubble Space Telescope, we have resolved individual red-giant branch stars in the halos of eight nearby spiral galaxies. The fields lie at projected distances between 2 and 13 kpc along the galaxies' minor axes. The data set…

Astrophysics · Physics 2009-11-13 M. Mouhcine , H. C. Ferguson , R. M. Rich , T. M. Brown , T. E. Smith

2MASS K_S band data of the inner 60 pc of the Galaxy are used to reconstruct the line-of-sight distances of the giant molecular clouds located in this region. Using the 2MASS H band image of the same region, two different populations of…

Astrophysics · Physics 2009-11-07 B. Vollmer , R. Zylka , W. J. Duschl

An object discovered during an infrared survey of the field near the quasar B2 0149+33 has an emission line at 2.25$\mu$m that we interpret as H$\alpha$ at a redshift of 2.43. The K-band image shows two compact components 10 kpc apart…

Astrophysics · Physics 2009-10-30 S. V. W. Beckwith , D. Thompson , F. Mannucci , S. G. Djorgovski

We present an analysis of the dust optical properties at large scale, for the whole galactic anticenter hemisphere. We used the 2MASS Extended Source Catalog to obtain the total reddening on each galaxy line of sight and we compared this…

Astrophysics · Physics 2009-10-19 L. Cambresy , T. H. Jarrett , C. A. Beichman

Space reddenings are derived for 15 Galactic Cepheids from dereddening CCD BVRIc data for AF-type stars in the immediate vicinities of the variables, in conjunction with 2MASS reddenings for BAF-type stars in the same fields. Potential…

Solar and Stellar Astrophysics · Physics 2011-07-08 David G. Turner , Ryan F. MacLellan , Arne A. Henden , Leonid N. Berdnikov

We present the first color-magnitude study for Palomar 2, a distant and heavily obscured globular cluster near the Galactic anticenter. Our (V,V-I) color-magnitude diagram (CMD), obtained with the UH8K camera at the CFHT, reaches V(lim) =…

Astrophysics · Physics 2009-10-30 W. E. Harris , P. R. Durrell , G. R. Petitpas , T. M. Webb , S. C. Woodworth

We use the VVV survey observations in bulge regions close to the Galactic plane to trace the bar inclination at the Galactic latitude b\sim\pm1{\deg} and to investigate a distinct structure in the inner regions of the bar that was…

Astrophysics of Galaxies · Physics 2015-05-30 O. A. Gonzalez , M. Rejkuba , D. Minniti , M. Zoccali , E. Valenti , R. K. Saito
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