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相关论文: An Inner Molecular Bar or Disk in NGC 5195

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We have mapped the central region of the Seyfert 1 galaxy NGC 1097 in 12CO(J=2-1) with the Submillieter Array (SMA). The 12CO(J=2-1) map shows a central concentration and a surrounding ring, which coincide respectively with the Seyfert…

天体物理学 · 物理学 2009-11-13 Pei-Ying Hsieh , Satoki Matsushita , Jeremy Lim , Kotaro Kohno , Satoko Sawada-Satoh

The Seyfert galaxy NGC 1097 has an extended neutral hydrogen disk, a companion, a prominent bar and a luminous circumnuclear starburst "ring". Magnetic fields as revealed by nonthermal radio-continuum emissions correlate well with the…

天体物理学 · 物理学 2009-11-06 Yu-Qing Lou , ZuHui Fan , Chi Yuan , Stephane Leon

NGC 1808 is a nearby barred starburst galaxy with an outflow from the nuclear region. To study the inflow and outflow processes related to star formation and dynamical evolution of the galaxy, we have carried out \(^{12}\)CO (\(J=1-0\))…

星系天体物理 · 物理学 2016-06-01 Dragan Salak , Naomasa Nakai , Takuya Hatakeyama , Yusuke Miyamoto

We present new J=1-0 12-CO observations along the northern spiral arm of the grand-design spiral galaxy M100 (NGC 4321), and study the distribution of molecular hydrogen as derived from these observations, comparing the new data with a set…

天体物理学 · 物理学 2007-05-23 J. H. Knapen , J. E. Beckman , J. Cepa , N. Nakai

We report high-resolution CO(1-0) observations in the central 6 kpc of the LINER galaxy NGC 5005 with the Owens Valley Radio Observatory millimeter array. Molecular gas is distributed in three components - a ring at a radius of about 3 kpc,…

天体物理学 · 物理学 2009-10-31 Kazushi Sakamoto , Andrew J. Baker , Nick Z. Scoville

The nucleus of the box-shaped galaxy NGC4013 has been observed with the IRAM interferometer in the J=1-0 and J=2-1 lines of 12CO. Our maps show the existence of a fast--rotating(130 km/s) molecular gas disk of radius r=110pc. Several…

天体物理学 · 物理学 2008-11-26 S. Garcia-Burillo , F. Combes , R. Neri

We have initiated the first CO interferometer survey of early-type spiral galaxies (S0-Sab). We observed five early-type spiral galaxies with HII nuclei (indicating circumnuclear starburst activities). These observations indicate gas masses…

天体物理学 · 物理学 2009-11-10 J. Koda , T. Okuda , K. Nakanishi , K. Kohno , S. Ishizuki , N. Kuno , S. K. Okumura

By image processing and color excess analyses of B, V, R, and I-band CCD images of the central region of M31 taken with the Kiso 105-cm Schmidt telescope, we found a bar of 200 pc length. We also found a more extended ``face-on" spiral…

天体物理学 · 物理学 2007-05-23 Y. Sofue , S. Yoshida , T. Aoki , T. Soyano , M. Hamabe , K. Wakamatsu

The central 2x1 kpc of the starburst galaxy NGC 253 has been imaged using the Submillimeter Array at a 60 pc resolution in the J=2-1 transitions of 12CO, 13CO, and C18O as well as in the 1.3 mm continuum. Molecular gas and dust are mainly…

We investigate star formation at very early evolutionary phases in five massive clouds in the inner 500 pc of the Galaxy, the Central Molecular Zone. Using interferometer observations of H$_2$O masers and ultra-compact H II regions, we find…

Maps of the J=2-1 12CO emission from the SbII galaxy NGC 7331 show a low-contrast ring at a radius of about 3.5 kpc. There is no evidence for a pronounced central hole in the CO distribution as claimed by others. The molecular ring is just…

天体物理学 · 物理学 2007-05-23 F. P. Israel , F. Baas

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

The study of the gas kinematic in the central 1.5kpc x 1.5kpc region of M31 has revealed several surprises. The starting point of this investigation was the detection at the IRAM-30m telescope of molecular gas with very large line…

宇宙学与河外天体物理 · 物理学 2015-05-27 Anne-Laure Melchior , Francoise Combes

We report interferometric radio CO2-1 observations at a resolution of 0.7", and 0.085" resolution adaptive optics K-band spectroscopy of the inner few arcseconds of NGC7469. The CO2-1 map shows a ring of molecular clouds and a bright…

天体物理学 · 物理学 2009-11-10 R. Davies , L. Tacconi , R. Genzel

We present the highest resolution (1") $^{12}$CO(1-0) observations of molecular gas in the dwarf starburst galaxy NGC 625, to date, obtained with ALMA. Molecular gas is distributed in discrete clouds within an area of $0.4$ kpc$^2$ and does…

星系天体物理 · 物理学 2020-05-27 Nia Imara , Ilse De Looze , Christopher M. Faesi , Diane Cormier

We report high resolution 2" ~ 200 pc mappings of the central region of the nearby barred spiral galaxy NGC 1365 in the CO(1--0) and CO(2--1) emission lines. The 2--1/1--0 ratio of integrated intensities shows a large scatter (0.15) with a…

星系天体物理 · 物理学 2022-08-24 Fumi Egusa , Yulong Gao , Kana Morokuma-Matsui , Guilin Liu , Fumiya Maeda

New observations of CO (J=1->0) line emission from M33, using the 25 element BEARS focal plane array at the Nobeyama Radio Observatory 45-m telescope, in conjunction with existing maps from the BIMA interferometer and the FCRAO 14-m…

天体物理学 · 物理学 2011-02-11 E. Rosolowsky , E. Keto , S. Matsushita , S. Willner

We present Hubble Space Telescope photometry of young stars in NGC 5102, a nearby gas-rich post-starburst S0 galaxy with a bright young stellar nucleus. We use the IAC-pop/MinnIAC algorithm to derive the recent star formation history in…

宇宙学与河外天体物理 · 物理学 2015-05-18 Sylvie F. Beaulieu , Kenneth C. Freeman , Sebastian L. Hidalgo , Colin A. Norman , Peter J. Quinn

Observations of galaxies at sub-millimeter wavelengths, where the emission is mainly due to cold dust, are required to constrain the dust physical properties and provide important insight on the gas content of galaxies. We mapped NGC1365 at…

宇宙学与河外天体物理 · 物理学 2015-06-15 F. S. Tabatabaei , A. Weiss , F. Combes , C. Henkel , K. M. Menten , R. Beck , A. Kovács , R. Guesten

In this paper we present new measurements of the gas kinematics in M33 using the CO J=1-0 line. The resulting rotational velocities complement previous 21-cm line data for a very accurate and extended rotation curve. The implied dark matter…

天体物理学 · 物理学 2008-11-26 Edvige Corbelli