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相关论文: Central Spiral Structure of Molecular Gas in Maffe…

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We present a 9'x9' fully-sampled map of the CO J=1-0 emission in the nearby starburst galaxy Maffei 2 obtained at the Five College Radio Astronomy Observatory. The map reveals previously known strong CO emission in the central starburst…

天体物理学 · 物理学 2009-11-10 A. M. Mason , C. D. Wilson

(Abridged) We present resolution maps of CO, its isotopologues, and HCN from in the center of Maffei 2. The J=1-0 rotational lines of 12^CO, 13^CO, C18^O and HCN, and the J=2-1 lines of 13^CO and C18^O were observed with the OVRO and BIMA…

天体物理学 · 物理学 2009-11-13 David S. Meier , Jean L. Turner , Robert. L. Hurt

Using the IRAM interferometer we have mapped at high resolution (2"x1") the 12CO(1-0) emission in the nucleus of the doubled barred SABbc spiral M100. Molecular gas is distributed in a two spiral arm structure starting from the end points…

天体物理学 · 物理学 2016-08-30 S. Garcia-Burillo , M. J. Sempere , F. Combes , R. Neri

We present J=2-1, J=3-2, J=4-3 12CO and 492 GHz [CI] maps as well as J=2-1 and J=3-2 13CO measurements of the central regions in the nearby Sc galaxies IC 342 and Maffei 2. In both galaxies, the distribution of CO and [CI] is strongly…

天体物理学 · 物理学 2009-11-07 F. P. Israel , F. Baas

We present the results of high-resolution 13CO(1-0) mapping observations with the NRO 45m telescope of the area toward the southern bright arm region of M51, including the galactic center. The obtained map shows the central depression of…

天体物理学 · 物理学 2015-06-24 T. Tosaki , T. Hasegawa , Y. Shioya , N. Kuno , S. Matsushita

We present CO(1-0) and CO(2-1) observations of the SA(rs)bc Seyfert 2 galaxy NGC 3147, obtained with the IRAM interferometer at 1\farcs9 $\times$1\farcs6 and 1\farcs6 $\times$1\farcs4 resolutions, respectively. A central peak seen mainly in…

天体物理学 · 物理学 2009-11-13 V. Casasola , F. Combes , S. Garcia-Burillo , L. K. Hunt , S. Leon , A. J. Baker

We study the molecular gas properties in the central kiloparsec of 29 barred and 15 unbarred spirals from the BIMA Survey of Nearby Galaxies (SONG). We find that the mean nuclear molecular gas surface density of barred spirals…

天体物理学 · 物理学 2007-05-23 Kartik Sheth

We present the kinematics of the molecular gas in the barred spiral galaxy M83 (NGC5236). The study is based on ^{12}CO(J=1--0 and 2--1) observations with the Swedish-ESO Submillimetre Telescope (SEST). Iso-velocity maps of the entire…

天体物理学 · 物理学 2009-11-10 A. A. Lundgren , H. Olofsson , T. Wiklind , G. Rydbeck

We compare the distribution of molecular gas and star formation activity in the bar region of six spirals (NGC 2903, NGC 3627, NGC 4321, NGC 5457, NGC 6946, & IC 342) from the BIMA Survey of Nearby Galaxies (SONG). The molecular gas, traced…

We present high spatial resolution (1.2") mm-interferometric observations of the CO(2-1) line emission in the central 300pc of the late-type spiral galaxy IC342. The data, obtained with the Owens Valley Radio Observatory, allow first-time…

天体物理学 · 物理学 2009-11-07 E. Schinnerer , T. Boeker , D. S. Meier

We present CO(1-0) and CO(2-1) Swedish-ESO Submillimetre Telescope (SEST) observations of the barred spiral galaxy M83 (NGC5236). The maps cover the entire optical disk. The CO emission is strongly peaked toward the nucleus, which breaks up…

天体物理学 · 物理学 2009-11-10 A. A. Lundgren , T. Wiklind , H. Olofsson , G. Rydbeck

Nearby galaxies exhibit a variety of structures, including central rings, similar to the MW Central Molecular Zone (CMZ). These rings are common in barred galaxies and can be gas-rich and highly star-forming. We aim to study molecular gas…

The structures and dynamics of the interstellar medium are governed by a combination of self-gravity, external gravity, and various sources of ordered and random motions on different spatial scales. This paper uses ALMA CO (3-2)…

星系天体物理 · 物理学 2026-04-27 Liam M. Wang , Jiayi Sun , Yu-Hsuan Teng , Eric W. Koch , Sanghyuk Moon , Elias Oakes , Erik Rosolowsky

The NRO/OVRO imaging survey of molecular gas in 20 spiral galaxies is used to test the theoretical predictions on bar-driven gas transport, bar dissolution, and bulge evolution. In most galaxies in the survey we find gas condensations of…

天体物理学 · 物理学 2007-05-23 K. Sakamoto , S. K. Okumura , S. Ishizuki , N. Z. Scoville

We present new interferometer observations of the 12CO(1-0) and 12CO(2-1) line emission of NGC 1068 with a resolution of 0.7''. The molecular gas in the inner 5'' is resolved into a ring with two bright knots east and west of the nuclear…

天体物理学 · 物理学 2009-10-31 E. Schinnerer , A. Eckart , L. J. Tacconi , R. Genzel , D. Downes

Previous molecular gas observations at arcsecond-scale resolution of the Seyfert 2 galaxy M51 suggest the presence of a dense circumnuclear rotating disk, which may be the reservoir for fueling the active nucleus and obscures it from direct…

天体物理学 · 物理学 2010-05-25 Satoki Matsushita , Sebastien Muller , Jeremy Lim

The center of M83, a barred starburst galaxy with a double nucleus, has been observed in the CO(J=2-1) and CO(J=3-2) lines with the Submillimeter Array. The molecular gas shows a distribution and kinematics typical for barred galaxies at…

天体物理学 · 物理学 2009-11-10 Kazushi Sakamoto , Satoki Matsushita , Alison B. Peck , Martina C. Wiedner , Daisuke Iono

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 ALMA observations of the most massive (star forming) galaxy in the redshift range 3<z<4 within the whole GOODS-S field. We detect a large elongated structure of molecular gas around the massive primeval galaxy, traced by the…

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…

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