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相关论文: Probing the interstellar medium of NGC1569 with He…

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We used the near-IR imager/spectrograph LUCIFER mounted on the Large Binocular Telescope (LBT) to image, with sub-arcsec seeing, the local dwarf starburst NGC 1569 in the JHK bands and HeI 1.08 micron, [FeII] 1.64 micron and Brgamma…

We present new 450 and 850 microns SCUBA data of the dwarf galaxy NGC 1569. We construct the mid-infrared to millimeter SED of NGC 1569, using ISOCAM, ISOPHOT, IRAS, KAO, SCUBA and MAMBO data, and model the SED in order to explore the…

天体物理学 · 物理学 2009-11-07 F. Galliano , S. C. Madden , A. P. Jones , C. D. Wilson , J. -P. Bernard , F. Le Peintre

We present near-IR JH spectra of the central regions of the dwarf starburst galaxy NGC 1569 using the Florida Image Slicer for Infrared Cosmology and Astrophysics (FISICA). The dust-penetrating properties and available spectral features of…

宇宙学与河外天体物理 · 物理学 2015-06-11 D. M. Clark , S. S. Eikenberry , S. N. Raines , N. Gruel , R. Elston , R. Guzman , G. Boreman , P. E. Glenn

We analyse multi-wavelength Hubble Space Telescope (HST) observations of a large number of star clusters in the nearby (post-) starburst dwarf galaxy NGC 1569. Their spectral energy distributions (SEDs) cover at least the wavelength range…

天体物理学 · 物理学 2009-11-10 P. Anders , R. de Grijs , U. Fritze--v. Alvensleben , N. Bissantz

We used a data set from AKARI and Herschel images at wavelengths from 7 $\mu$m to 500 $\mu$m to catch the evidence of dust processing in galactic winds in NGC 1569. Images show a diffuse infrared (IR) emission extending from the galactic…

We present the results from an analysis of deep Herschel Space Observatory observations of six nearby dwarf galaxies known to host galactic-scale winds. The superior far-infrared sensitivity and angular resolution of Herschel have allowed…

We report Keck-NIRSPEC observations of the Brackett $\alpha$ 4.05 $\mu$m recombination line across the two candidate embedded super star clusters (SSCs) in NGC 1569. These SSCs power a bright HII region and have been previously detected as…

星系天体物理 · 物理学 2021-03-05 Daniel P. Cohen , Jean L. Turner , Sara C. Beck , S. Michelle Consiglio

We present deep WIYN H-alpha imaging of the dwarf irregular starburst galaxy NGC 1569, together with WIYN SparsePak spatially-resolved optical spectroscopy of the galactic outflow. This leads on from our previous detailed analyses of the…

天体物理学 · 物理学 2009-11-13 M. S. Westmoquette , L. J. Smith , J. S. Gallagher

We present a set of four Gemini-North GMOS/IFU observations of the central disturbed regions of the dwarf irregular starburst galaxy NGC 1569, surrounding the well-known super star clusters A and B. This continues on directly from a…

天体物理学 · 物理学 2009-11-13 M. S. Westmoquette , L. J. Smith , J. S. Gallagher , K. M. Exter

We investigate spatial the distribution of the intrinsic extinction in the starburst dwarf galaxy NGC1569 creating an extinction map of the whole galaxy derived from the Halpha/Hbeta emission line ratio. We differentiate the extinction in…

天体物理学 · 物理学 2007-05-23 M. Relano , U. Lisenfeld , J. M. Vilchez , E. Battaner

We are modeling the spectra of dwarf galaxies from infrared to submillimeter wavelengths to understand the nature of the various dust components in low-metallicity environments, which may be comparable to the ISM of galaxies in their early…

天体物理学 · 物理学 2015-06-24 F. Galliano , S. C. Madden , A. P. Jones , C. D. Wilson , J. -P. Bernard , F. Le Peintre

In order to understand the formation and evolution of dIm galaxies, one needs to understand their three-dimensional structure. We present measurements of the stellar velocity dispersion in NGC 1569, a nearby post-starburst dIm galaxy. The…

宇宙学与河外天体物理 · 物理学 2013-04-03 Megan Johnson , Deidre A. Hunter , Se-Heon Oh , Hong-Xin Zhang , Bruce Elmegreen , Elias Brinks , Erik Tollerud , Kimberly Herrmann

We present a far-ultraviolet (FUV) analysis of the star-forming complexes (SFCs) in the nearby spiral galaxy NGC\,2090, based on observations from the Ultraviolet Imaging Telescope (UVIT), and compare it with emission from the optical and…

星系天体物理 · 物理学 2026-05-13 Jyoti Yadav , Mousumi Das , S Amrutha , Dimitra Rigopoulou

We present H- and K-band NIRSPEC spectroscopy of super star clusters (SSCs) in the irregular starburst galaxy NGC 1569, obtained at the Keck Observatory. We fit these photospheric spectra to NextGen model atmospheres to obtain effective…

天体物理学 · 物理学 2007-05-23 Andrea M. Gilbert , James R. Graham

We investigate the distribution of the intrinsic extinction in NGC1569 using an extinction map derived from the H_alpha/H_beta emission line ratio. We compare the extinction distribution to that of the dust emission traced by SPITZER…

天体物理学 · 物理学 2009-11-11 M. Relano , U. Lisenfeld , E. Battaner , J. M. Vilchez , P. Perez-Gonzalez

(abridged) We used HST/ACS to obtain deep V- and I-band images of NGC 1569, one of the closest and strongest starburst galaxies in the Universe. These data allowed us to study the underlying old stellar population, aimed at understanding…

We present new results on the star formation history of the dwarf irregular galaxy NGC 1569. The data were obtained with Hubble Space Telescope's NICMOS/NIC2 in the F110W (J) and F160W (H) near-infrared (NIR) filters and interpreted with…

天体物理学 · 物理学 2009-11-11 L. Angeretti , M. Tosi , L. Greggio , E. Sabbi , A. Aloisi , Claus Leitherer

To assess the effects of the cluster environment on the different components of the interstellar medium, we analyse the FIR-submm properties of a sample of star-forming dwarf (SFD) galaxies detected by the Herschel Virgo Cluster Survey…

We present new data of the dwarf galaxy NGC 1569 at 450 $\mu$m, 850 $\mu$m and 1200$\mu$m taken with SCUBA at the JCMT and the bolometer array at the IRAM 30m telescope. After including data from IRAS at 12, 25, 60 and 100 $\mu$m, we have…

天体物理学 · 物理学 2016-08-30 U. Lisenfeld , F. P. Isreal , J. M. Stil , A. Sievers

We present the results from an analysis of deep Herschel far-infrared observations of the edge-on disk galaxy NGC 3079. The PSF-cleaned PACS images at 100 and 160 um display a 25 kpc x 25 kpc X-shape structure centered on the nucleus that…

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