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相关论文: A distant OB association around RAFGL 5475

200 篇论文

We present a JHKL survey of the massive star forming region RCW 57 (NGC 3576) based on L-band data at 3.5 micron taken with SPIREX (South Pole Infrared Explorer), and 2MASS JHK data at 1.25-2.2 micron. This is the second of two papers, the…

天体物理学 · 物理学 2009-11-11 M. Maercker , M. G. Burton , C. M. Wright

By means of different physical mechanisms, the expansion of HII regions can promote the formation of new stars of all masses. RCW 120 is a nearby Galactic HII region where triggered star formation occurs. This region is well-studied - there…

A 0.35\degr $\times$ 0.29\degr field centered at $l$=--18.63\degr, $b$=0.35\degr was observed during the ISOGAL survey by ISOCAM imaging at 7$\mu$m and 15{\rm $\mu$m}. 648 objects were detected and their brightness are measured. By…

天体物理学 · 物理学 2011-05-23 B. W. Jiang , A. Omont , S. Ganesh , G. Simon , F. Schuller

We have carried out a near-infrared imaging survey of luminous young stellar outflow candidates using the United Kingdom Infrared Telescope. Observations were obtained in the broad band K (2.2 mu) and through narrow band filters at the…

太阳与恒星天体物理 · 物理学 2015-05-18 Watson P. Varricatt , Christopher J. Davis , Suzanne Ramsay , Stephen P. Todd

We present the first results of a comprehensive census of the stellar content of the nearby OB associations based on Hipparcos positions, proper motions and parallaxes for 12842 candidate member stars distributed over 21 fields on the sky.…

天体物理学 · 物理学 2007-05-23 P. T. de Zeeuw , A. G. A. Brown , J. H. J. de Bruijne , R. Hoogerwerf , J. Lub , R. S. Le Poole , A. Blaauw

We present a near infrared study of the stellar content of 35 H\,{\sc{ii}} regions in the Galactic plane. In this work, we have used the near infrared domain $J-$, $H-$ and $K_{s}-$ band color images to visually inspect the sample. Also,…

太阳与恒星天体物理 · 物理学 2015-05-20 A. P. Moisés , A. Damineli , E. Figuerêdo , R. D. Blum , P. S. Conti , C. L. Barbosa

We present initial results of the first panoramic search for high-amplitude near-infrared variability in the Galactic Plane. We analyse the widely separated two-epoch K-band photometry in the 5th and 7th data releases of the UKIDSS Galactic…

We present mid-infrared maps and preliminary analysis for 61 galaxies observed with the ISOCAM instrument aboard the Infrared Space Observatory. Many of the general features of galaxies observed at optical wavelengths---spiral arms, disks,…

天体物理学 · 物理学 2009-10-31 Daniel A. Dale , Nancy A. Silbermann , George Helou

The Quintuplet, one of three massive stellar clusters in the Galactic center, is located about 30pc in projection from Sagittarius A*. Based on near-infrared K-band spectra we determine temperatures and luminosities for all stars in our…

星系天体物理 · 物理学 2012-03-13 A. Liermann , W. -R. Hamann , L. M. Oskinova

Context. With the latest infrared surveys, the number of massive protostellar candidates has increased significantly. New studies have posed additional questions on important issues about the formation, evolution, and other phenomena…

星系天体物理 · 物理学 2015-05-19 P. Benaglia , M. Ribo , J. A. Combi , G. E. Romero , S. Chaty , B. Koribalski , I. F. Mirabel , L. F. Rodriguez , G. Bosch

An analysis of low resolution spectra and infared data of 29 ISOGAL-DENIS sources with mid-IR excess is presented. Eight ISOGAL sources from our sample with 7-15 micron excess are found to be B and A-type stars, some of them with emission…

天体物理学 · 物理学 2009-11-07 M. Schultheis , M. Parthasarathy , A. Omont , M. Cohen , S. Ganesh , F. Sevre , G. Simon

This first part of Special Session 5 explored the current status of infrared-based observations of obscured and distant stellar clusters in the Milky Way galaxy. Recent infrared surveys, either serendipitously or using targeted searches,…

太阳与恒星天体物理 · 物理学 2012-10-16 M. M. Hanson , D. Froebrich , F. Martins , A. -N. Chene , C. Rosslowe , A. Herrero , H. -J. Kim

We present follow-up spectroscopy on a protocluster candidate selected from the wide-field imaging of the Hyper SuprimeCam Subaru Strategic Programme. The target protocluster candidate was identified as a $4.5\sigma$ overdense region of…

We present the discovery of four remote star clusters in M33, one of which is of an extended nature. Three of the clusters were discovered using survey data from the Isaac Newton Telescope Wide-Field Camera while one was discovered…

宇宙学与河外天体物理 · 物理学 2011-02-11 A. Huxor , A. M. N. Ferguson , M. K. Barker , N. R. Tanvir , M. J. Irwin , S. C. Chapman , R. Ibata , G. Lewis

We have studied the properties of an infrared cluster embedded in the gas and dust of the southern part of the Carina Nebula (NGC 3372), where the probable existence of current star formation has already been predicted. We used mid-infrared…

天体物理学 · 物理学 2009-11-10 G. F. Hägele , J. F. Albacete Colombo , R. H. Barbá , G. L. Bosch

We report on our search for distant clusters of galaxies based on optical and X-ray follow up observations of X-ray candidates from the SHARC survey. Based on the assumption that the absence of bright optical or radio counterparts to…

天体物理学 · 物理学 2009-11-13 C. Adami , M. P. Ulmer , F. Durret , G. Covone , E. Cypriano

We aim to investigate the global star formation scenario in star-forming sites AFGL 5157, [FSR2007] 0807 (hereafter FSR0807), [HKS2019] E70 (hereafter E70), [KPS2012] MWSC 0620 (hereafter KPS0620), and IRAS 05331+3115 in the outer galactic…

We have discovered an optically rich galaxy cluster at z=1.7089 with star formation occurring in close proximity to the central galaxy. The system, SpARCS104922.6+564032.5, was detected within the Spitzer Adaptation of the red-sequence…

We present an analysis of the optical spectroscopy of 58 stars in the Galactic plane at $l=27$\arcdeg, where a prominent excess in the flux distribution and star counts have been observed in several spectral regions, in particular in the…

天体物理学 · 物理学 2009-10-30 F. Garzon , M. Lopez-Corredoira , P. Hammersley , T. J. Mahoney , X. Calbet , J. E. Beckman

We present far-infrared observations of Monoceros R2 (a giant molecular cloud at approximately 830 pc distance, containing several sites of active star formation), as observed at 70 {\mu}m, 160 {\mu}m, 250 {\mu}m, 350 {\mu}m, and 500 {\mu}m…