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相关论文: IC 10: More evidence that it is a blue compact dwa…

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A sample of 16 blue compact dwarf galaxies (BCDs) in the Virgo Cluster has been imaged in the near-infrared (NIR) in $J$ and $K_s$ on the 2.1m telescope at OAN-SPM in Mexico. Isophotes as faint as $\mu_J$ = 24 mag arcsec$^{-2}$ and…

天体物理学 · 物理学 2008-11-26 O. Vaduvescu , M. G. Richer , M. L. McCall

White dwarfs whose atmospheres are polluted by terrestrial-like planetary debris have become a powerful and unique tool to study evolved planetary systems. This paper presents results for an unbiased Spitzer IRAC search for circumstellar…

地球与行星天体物理 · 物理学 2015-03-20 M. Rocchetto , J. Farihi , B. T. Gaensicke , C. Bergfors

Using HST NICMOS 2 observations we have measured 1.6-micron near infrared nuclear luminosities of 100 3CR radio galaxies with z<0.3, by modeling and subtracting the extended emission from the host galaxy. We performed a multi-wavelength…

宇宙学与河外天体物理 · 物理学 2015-05-20 R. D. Baldi , M. Chiaberge , A. Capetti , W. Sparks , F. D. Macchetto , C. P. O'Dea , D. J. Axon , S. A. Baum , A. C. Quillen

We present 4-micron ISAAC imaging and spectroscopy of the extremely metal-poor dwarf galaxy SBS 0335-052, aimed at a better understanding of the dust in this low-metallicity galaxy. The 4-micron emission turns out to be very compact,…

天体物理学 · 物理学 2009-11-07 L. K. Hunt , L. Vanzi , T. X. Thuan

Hubble Space Telescope (HST) colour - magnitude diagrams in B, V and R along with long-slit Multiple Mirror Telescope (MMT) spectrophotometric data are used to investigate the evolutionary status of the nearby blue compact dwarf (BCD)…

天体物理学 · 物理学 2007-05-23 Y. I. Izotov , P. Papaderos , T. X. Thuan , K. J. Fricke , C. B. Foltz , N. G. Guseva

We present preliminary results from a study of the compact star cluster populations in three local luminous blue compact galaxies: ESO 185-IG 013, ESO 350-IG 038 (a.k.a. Haro 11), and MRK 930. These systems show peculiar morphologies and…

宇宙学与河外天体物理 · 物理学 2009-07-20 Angela Adamo , Göran Östlin , Erik Zackrisson , Matthew Hayes

Far-ultraviolet spectra obtained with $FUSE$ show that the strong $CII\lambda$1036 interstellar absorption-line is essentially black in five of the UV-brightest local starburst galaxies. Since the opacity of the neutral ISM below the…

天体物理学 · 物理学 2009-11-06 T. Heckman , K. R. Sembach , G. Meurer , C. Leitherer , D. Calzetti , C. L. Martin

[abridged] We present 52-93 micron spectra obtained with Spitzer in the MIPS-SED mode, of a representative sample of luminous compact far-IR sources in the LMC. These include carbon stars, OH/IR AGB stars, post-AGB objects and PNe,…

The nature of possible evolutionary pathways between various types of dwarf galaxies is still not fully understood. Blue compact dwarf galaxies (BCDs) provide a unique window into dwarf galaxy formation and evolution and are often thought…

星系天体物理 · 物理学 2014-10-28 Steven Janowiecki , John J. Salzer

The Fornax cluster galaxy FCC 35 shows an unusual multiply-peaked integrated HI profile (Bureau, Mould & Staveley-Smith 1996). We have now observed FCC 35 with the Australia Telescope Compact Array (ATCA) and have found a compact HI source…

天体物理学 · 物理学 2007-05-23 M. E. Putman , M. Bureau , J. R. Mould , L. Staveley-Smith , K. C. Freeman

We have used observations of the galaxy IC 10 at the 6-m telescope of the Special Astrophysical Observatory with the SCORPIO focal reducer in the Fabry-Perot interferometer mode and with the MPFS spectrograph to study the structure and…

宇宙学与河外天体物理 · 物理学 2010-12-13 O. V. Egorov , T. A. Lozinskaya , A. V. Moiseev

We present 11.7-micron observations of nine late-type dwarfs obtained at the Keck I 10-meter telescope in December 2002 and April 2003. Our targets were selected for their youth or apparent IRAS 12-micron excess. For all nine sources,…

天体物理学 · 物理学 2009-11-11 Peter Plavchan , M. Jura , S. J. Lipscy

Extensive photometric studies of the globular clusters located towards the center of the Milky Way have been historically neglected. The presence of patchy differential reddening in front of these clusters has proven to be a significant…

We report spectra obtained with the Spitzer Space Telescope in the wavelength range between 14 microns and 35 microns of 19 nearby main-sequence stars with infrared excesses. The six stars with strong dust emission show no recognizable…

We have obtained near-infrared images and mid-infrared spectra of the starburst core of the dwarf Wolf-Rayet galaxy He 2-10. We find that the infrared continuum and emission lines are concentrated in a flattened ellipse 3-4'' or 150 pc…

天体物理学 · 物理学 2009-10-30 S. C. Beck , D. M. Kelly , J. H. Lacy

"Cometary" Blue Compact Dwarf Galaxies (iI,C BCDs) are characterized by off-center starbursts close to the end of an elongated dwarf irregular (dI)-like host galaxy. This may either represent randomly enhanced star-forming activity of a dI,…

天体物理学 · 物理学 2007-05-23 K. G. Noeske , N. G. Guseva , K. J. Fricke , Y. I. Izotov , P. Papaderos , T. X. Thuan

The metal deficient (Z = Z_sun/41) Blue Compact Dwarf Galaxy (BCD) SBS 0335-052 was observed with ISOCAM between 5 and 17 mic. With a L_12mic/L_B ratio of 2.15, the galaxy is unexpectedly bright in the mid-infrared for such a…

天体物理学 · 物理学 2009-10-31 T. X. Thuan , M. Sauvage , S. Madden

We report the discovery of SDSSJ1049+5103, an overdensity of resolved blue stars at (\alpha_{2000}, \delta_{2000}) = (162.343, 51.051). This object appears to be an old, metal-poor stellar system at a distance of 45 +/- 10 kpc, with a…