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相关论文: Multiwavelength study of the starburst galaxy NGC7…

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We combine existing multiwavelength data (incl. an HST/GHRS UV spectrum, an optical spectrum, far-IR, Xray and radio fluxes) with new HST/WFPC2 images, near-IR photometry and K band spectroscopy. We use these data to constrain the young,…

天体物理学 · 物理学 2016-08-30 Ariane Lancon , Jeff D. Goldader , Claus Leitherer , Rosa M. Gonzalez Delgado

We have obtained a Hubble Space Telescope ultraviolet image and spectrum of the nearby Wolf-Rayet galaxy NGC 1741. The spatial morphology from the Faint Object Camera image is dominated by two main starburst centers, each being about 100…

天体物理学 · 物理学 2009-10-28 Peter S. Conti , Claus Leitherer , William D. Vacca

We study the central (inner few hundred parsecs) stellar populations of four starburst galaxies (NGC34, NGC1614, NGC3310 and NGC7714) in the near-infrared (NIR), from 0.8 to 2.4microns, by fitting combinations of stellar population models…

天体物理学 · 物理学 2009-11-13 R. Riffel , M. G. Pastoriza , A. Rodriguez-Ardila , C. Maraston

We present the results of deep high resolution imaging performed with ACS/HRC@HST in the most active region of the nearby starburst galaxy NGC 4214. We resolved the stellar populations of five Young Massive Clusters and their surrounding…

星系天体物理 · 物理学 2015-06-17 A. Sollima , M. Cignoni , R. G. Gratton , M. Tosi , A. Bragaglia , S. Lucatello , G. Meurer

We present results from Chandra and XMM-Newton X-ray observations of NGC 4214, a nearby dwarf starburst galaxy containing several young regions of very active star-formation. Starburst regions are known to be associated with diffuse X-ray…

We have obtained high-spatial resolution ultraviolet and optical STIS spectroscopy and imaging of the metal-rich nuclear starburst in NGC3049. The stellar continuum and the absorption line spectrum in the ultraviolet are used to constrain…

天体物理学 · 物理学 2009-11-07 Rosa M. Gonzalez Delgado , Claus Leitherer , Grazyna Stasinka , Timothy Heckman

We present the results of an infrared photometric survey performed with NICS@TNG in the nearby starburst galaxy NGC 4214. We derived accurate integrated JK magnitudes of 10 young massive clusters and compared them with the already available…

宇宙学与河外天体物理 · 物理学 2015-06-15 A. Sollima , R. G. Gratton , E. Carretta , A. Bragaglia , S. Lucatello

We present first results of near-infrared integral field spectroscopy of the central 8''$\times$8'' of the Wolf-Rayet nucleus of the barred spiral galaxy NGC 6764. In addition to stellar CO and Na I absorption lines as well as recombination…

天体物理学 · 物理学 2007-05-23 A. Eckart , E. Schinnerer

We present an original study of the dwarf starburst galaxy NGC 4214. We use archival optical and UV images obtained with WFPC2 and STIS on-board the Hubble Space Telescope. We explain the process followed to obtain high-quality photometry…

天体物理学 · 物理学 2007-08-28 Leonardo Ubeda

(Abridged) We have performed a comprehensive multiwavelength analysis of a sample of 20 starburst galaxies that show the presence of a substantial population of massive stars. The main aims are the study of the massive star formation and…

天体物理学 · 物理学 2011-08-31 Angel R. Lopez-Sanchez , Cesar Esteban

We present observations of a massive star cluster near the nuclear region of the nearby starburst galaxy NGC 253. The peak of near-infrared emission, which is spatially separated by 4" from the kinematic center of the galaxy, is coincident…

太阳与恒星天体物理 · 物理学 2010-01-15 Katherine A. Kornei , Nate McCrady

NGC 7582 is defined as a Starburst/AGN galaxy, since its optical and X-Ray spectra reveal both characteristics. In this work, we show the results of a stellar population modeling in a datacube taken with the Gemini South telescope. We found…

宇宙学与河外天体物理 · 物理学 2015-05-18 T. V. Ricci , J. E. Steiner , R. B. Menezes , A. Garcia-Rissmann , R. Cid Fernandes

The interacting system Arp 284 consisting of the Wolf-Rayet galaxy NGC 7714 and its irregular companion NGC 7715 was observed using the Infrared Space Observatory. Deconvolved ISOCAM maps of the galaxies using the 14.3, 7.7 and 15 micron…

天体物理学 · 物理学 2007-05-23 B. O'Halloran , L. Metcalfe , M. Delaney , B. McBreen , R. Laureijs , K. Leech , D. Watson , L. Hanlon

Preliminary results from spectrophotometric observations of galaxies with very young starbursts are presented. Starburst galaxies with an age of the burst in the range between 3 and 6 Myr have been observed and new detections of Wolf-Rayet…

天体物理学 · 物理学 2007-05-23 Thierry Contini

We present the results of a detailed UV-optical study of the nearby dwarf starburst galaxy NGC 4214 using multifilter HST/WFPC2+STIS photometry. The stellar extinction is found to be quite patchy, with some areas having values of…

天体物理学 · 物理学 2009-06-23 Leonardo Úbeda , J. Maíz-Apellániz , John MacKenty

The modest extinction and reasonably face-on viewing geometry make the luminous IR galaxy NGC1614 an ideal laboratory for study of a powerful starburst. HST/NICMOS observations show: 1.) deep CO stellar absorption, tracing a starburst…

天体物理学 · 物理学 2009-10-31 A. Alonso-Herrero , C. W. Engelbracht , M. J. Rieke , G. H. Rieke , A. C. Quillen

We present observations of the starburst galaxy NGC 7714 with the Infrared Spectrograph IRS on board the Spitzer Space Telescope. The spectra yield a wealth of ionic and molecular features that allow a detailed characterization of its…

We employ the NASA Infrared Telescope Facility's near-infrared spectrograph SpeX at 0.8-2.4$\mu$m to investigate the spatial distribution of the stellar populations (SPs) in four well known Starburst galaxies: NGC34, NGC1614, NGC3310 and…

We present an analysis of late-time Hubble Space Telescope Wide Field Camera 3 and Wide Field Planetary Camera 2 observations of the site of the Type Ic SN 2007gr in NGC 1058. The SN is barely recovered in the late-time WFPC2 observations,…

太阳与恒星天体物理 · 物理学 2016-09-27 Justyn Maund , Enrico Ramirez-Ruiz

We present the data and methods that we have used to perform a detailed UV-optical study of the nearby dwarf starburst galaxy NGC 4214 using multifilter HST/WFPC2+STIS photometry. We explain the process followed to obtain high-quality…

天体物理学 · 物理学 2009-06-23 Leonardo Úbeda , J. Maíz-Apellániz , John MacKenty
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