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Results of optical and NIR spectral and photometric observations of a sample of candidate double-barred galaxies are presented. Velocity fields and velocity dispersion maps of stars and ionized gas, continuum and emission-line images were…

天体物理学 · 物理学 2009-11-10 A. V. Moiseev , J. R. Valdes , V. H. Chavushyan

We present high-resolution CO, HCN, and 13CO maps of the inner arcminute of NGC 1068 made with the BIMA interferometer. Several features appear in the CO map which have not previously been observed: (1) a firm detection of CO line emission…

天体物理学 · 物理学 2007-05-23 Tamara T. Helfer , Leo Blitz

We present the first spatially resolved spectroscopic imaging observations of the 12CO(1-0) line emission in the central 2.5 kpc of the Seyfert 1 galaxy NGC4151, obtained with the IRAM Plateau de Bure Interferometer (PdBI). Most of the cold…

宇宙学与河外天体物理 · 物理学 2015-05-19 G. Dumas , E. Schinnerer , C. G. Mundell

We analyse new H-band integral-field unit observations of two galaxies at ~4 Mpc, using a principal components analysis of pixel spectra to probe their giant star content. In both galaxies, the signals arise in near-resolved point-like…

星系天体物理 · 物理学 2026-05-22 Russell J. Smith , Anastasia Gvozdenko

Observations of the CO J(1-0) 115 GHz and J(2-1) 230 GHz lines in comet C/1995 O1 (Hale-Bopp) were performed with the IRAM Plateau de Bure interferometer on 11 March, 1997. The observations were conducted in both single-dish (ON-OFF) and…

地球与行星天体物理 · 物理学 2010-11-02 D. Bockelée-Morvan , F. Henry , N. Biver , J. Boissier , P. Colom , J. Crovisier , D. Despois , R. Moreno , J. Wink

We report the detection of spatially extended CO 1-0 and 5-4 emission in the z=2.49 submillimeter galaxy (SMG) J123707+6214, using the Expanded Very Large Array and the Plateau de Bure Interferometer. The large molecular gas reservoir is…

We present observations of CO(3-2) and $^{13}$CO(3-2) emission near the supernebula in the dwarf galaxy NGC 5253, which contains one of the best examples of a potential globular cluster in formation. The 0.3" resolution images reveal an…

星系天体物理 · 物理学 2020-05-15 J. L. Turner , S. M. Consiglio , S. C. Beck , W. M. Goss , P. T. P. Ho , D. S. Meier , S. Silich , J. -H. Zhao

NGC 3393, a nearby Seyfert 2 galaxy with nuclear radio jets, large-scale and nuclear bars, and a posited secondary super massive black hole, provides an interesting laboratory to test the physics of inflows and outflows. Here we present and…

We present new high-resolution observations of the center of the late-type spiral M100 (NGC 4321) supplemented by 3D numerical modeling of stellar and gas dynamics, including star formation (SF). NIR imaging has revealed a stellar bar,…

天体物理学 · 物理学 2010-04-21 J. H. Knapen , J. E. Beckman , C. H. Heller , I. Shlosman , R. S. de Jong

With the Infrared Camera on board AKARI, we carried out near-infrared (2.5-5.0 micron) spectroscopy of the central kiloparsec region of the barred spiral galaxy, NGC1097, categorized as Seyfert 1 with a circumnuclear starburst ring. Our…

We present high resolution (3" - 5") observations of CO(1-0) and HCN(1-0) emission from the circumnuclear star forming ring in the barred spiral galaxy NGC 6951, a host of a type-2 Seyfert, using the Nobeyama Millimeter Array and 45 m…

天体物理学 · 物理学 2009-10-30 Kotaro Kohno , Ryohei Kawabe , Baltasar Vila-Vilaro

We report the detection of outflowing molecular gas in the center of the nearby (z=0.014) massive radio galaxy NGC6328. The radio core of the galaxy, PKS B1718-649, is identified as a Gigahertz Peaked Spectrum source with a compact (2 pc)…

We report the detection of a narrow Fe-K emission line in the Seyfert 1 galaxy NGC 5548 with the Chandra High-Energy Transmission Gratings. In the galaxy frame we measure a center energy of 6.40 \pm 0.03 keV, a FWHM of 4515 (+3525,-2645)…

天体物理学 · 物理学 2009-10-31 T. Yaqoob , I. M. George , K. Nandra , T. J. Turner , P. J. Serlemitsos , R. F. Mushotzky

We present spatially resolved integral field spectroscopic K-band data at a resolution of 0.13" (60pc) and interferometric CO(2-1) line observations of the prototypical merging system NGC6240. Despite the clear rotational signature, the…

宇宙学与河外天体物理 · 物理学 2015-05-19 H. Engel , R. I. Davies , R. Genzel , L. J. Tacconi , E. K. S. Hicks , E. Sturm , T. Naab , P. H. Johansson , S. J. Karl , C. E. Max , A. Medling , P. P. van der Werf

We discuss a model of the central source in Seyfert 1 galaxy NGC 5548. The model assumes a three phase disk structure consisting of a cold outer disk, a hot central disk constituting a Comptonizing X/gamma source, and an intermediate…

天体物理学 · 物理学 2007-05-23 P. Magdziarz , O. Blaes

The molecular components of three giant HII regions (NGC 5461, NGC 5462, NGC 5471) in the galaxy M101 are investigated with new observations from the James Clerk Maxwell Telescope, the NRAO 12-meter, and the Owens Valley millimeter array.…

天体物理学 · 物理学 2009-10-31 J. Giannakopoulou-Creighton , M. Fich , C. D. Wilson

We present the results of the wide-field $^{12}$CO (1--0) observations of the nearby barred galaxy M83 carried out with the Nobeyama Millimeter Array (NMA). The interferometric data are combined with the data obtained with the Nobeyama 45-m…

We present high-angular-resolution (1".5 - 5") interferometer observations of the \co emission in the central region of the SA(s)c galaxy NGC 4254. The observations were obtained using the Nobeyama Millimeter-wave Array (NMA) during the…

天体物理学 · 物理学 2015-06-24 Yoshiaki Sofue , Jin Koda , Hiroyuki Nakanishi , Makoto Hidaka

We present the results of near-infrared H- and K-band European Southern Observatory SINFONI integral field spectroscopy of the Seyfert galaxy NGC 1566. We investigate the central kpc of this nearby galaxy, concentrating on excitation…

星系天体物理 · 物理学 2015-11-04 S. Smajić , L. Moser , A. Eckart , G. Busch , F. Combes , S. García-Burillo , M. Valencia-S. , M. Horrobin

The Sb galaxy NGC 2841 was observed at the 6 m telescope of SAO RAS with the Multi-Pupil Field Spectrograph and at the 1 m telescope of SAO RAS with the long-slit spectrograph. An unresolved nucleus of NGC 2841 is shown to be chemically…

天体物理学 · 物理学 2007-05-23 O. K. Sil'chenko , V. V. Vlasyuk , A. N. Burenkov