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相关论文: Molecular gas and star formation in the red-sequen…

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We report the detection of 1 10^7 M_sun of molecular gas in the central region of the S0/E7 galaxy NGC4550, inferred from observations of CO(1-0) emission. Dust is detected in HST WFPC2 images and found to be asymmetrically distributed…

天体物理学 · 物理学 2009-11-06 T. Wiklind , C. Henkel

In order to try and understand its origins, we present high-quality long-slit spectral observations of the counter-rotating stellar discs in the strange S0 galaxy NGC 4550. We kinematically decompose the spectra into two counter-rotating…

宇宙学与河外天体物理 · 物理学 2015-06-11 Evelyn J. Johnston , Michael R. Merrifield , Alfonso Aragon-Salamanca , Michele Cappellari

We present interferometric observations resolving the CO emission in the four gas-rich lenticular galaxies NGC 3032, NGC 4150, NGC 4459, and NGC 4526, and we compare the CO distribution and kinematics to those of the stars and ionized gas.…

天体物理学 · 物理学 2009-11-13 Lisa M. Young , Martin Bureau , Michele Cappellari

We present the results of integral-field spectroscopic observations of the two disk galaxies NGC 3593 and NGC 4550 obtained with VIMOS/VLT. Both galaxies are known to host 2 counter-rotating stellar disks, with the ionized gas co-rotating…

宇宙学与河外天体物理 · 物理学 2015-06-11 L. Coccato , L. Morelli , A. Pizzella , E. M. Corsini , L. M. Buson , E. Dalla Bonta'

We present the detection of molecular gas using CO(1-0) line emission and follow up Halpha imaging observations of galaxies located in nearby voids. The CO(1-0) observations were done using the 45m telescope of the Nobeyama Radio…

星系天体物理 · 物理学 2014-11-10 M. Das , T. Saito , D. Iono , M. Honey , S. Ramya

ALMA imaging of the cold molecular medium in the nearby starburst galaxy NGC 1808 is presented. The observations reveal the distribution of molecular gas, traced by $^{12}$CO (1-0) and $^{12}$CO (3-2), and continuum (93 and 350 GHz) across…

星系天体物理 · 物理学 2017-11-15 Dragan Salak , Yuto Tomiyasu , Naomasa Nakai , Nario Kuno , Yusuke Miyamoto , Hiroyuki Kaneko

We present interferometric observations of CO lines (12CO(1-0, 2-1) and 13CO(1-0, 2-1)) and dense gas tracers (HCN(1-0), HCO+(1-0), HNC(1-0) and HNCO(4-3)) in two nearby edge-on barred lenticular galaxies, NGC 4710 and NGC 5866, with most…

星系天体物理 · 物理学 2016-09-21 Selcuk Topal , Martin Bureau , Timothy A. Davis , Melanie Krips , Lisa M. Young , Alison F. Crocker

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 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

IRAM 30m 12CO(1-0) and 12CO(2-1) HERA observations are presented for the ram-pressure stripped Virgo spiral galaxy NGC 4522. The CO emission is detected in the galactic disk and the extraplanar gas. The extraplanar CO emission follows the…

天体物理学 · 物理学 2009-11-13 B. Vollmer , J. Braine , C. Pappalardo , P. Hily-Blant

We present a high resolution (down to 0.18"), multi-transition imaging study of the molecular gas in the z = 4.05 submillimeter galaxy GN20. GN20 is one of the most luminous starburst galaxy known at z > 4, and is a member of a rich…

宇宙学与河外天体物理 · 物理学 2015-05-18 C. L. Carilli , E. Daddi , D. Riechers , F. Walter , A. Weiss , H. Dannerbauer , G. E. Morrison , J. Wagg , Romeel Dave , D. Elbaz , D. Stern , M. Dickinson , M. Krips , M. Aravena

Interferometric observations of the CO(1-0) line in the elliptical galaxy NGC759 shows that it contains 2 10^9 Mo of molecular gas, confined to a circumnuclear ring with an average radius of only 650pc. The maximum gas surface density is…

天体物理学 · 物理学 2007-05-23 Tommy Wiklind , Francoise Combes , Christian Henkel , Friedrich Wyrowski

Molecular gas plays a critical role in explaining the quiescence of star formation (SF) in massive isolated spiral galaxies, which could be a result of either the low molecular gas content and/or the low SF efficiency. We present IRAM 30m…

星系天体物理 · 物理学 2024-12-17 Yan Jiang , Jiang-Tao Li , Yu Gao , Joel N. Bregman , Li Ji , Xuejian Jiang , Qinghua Tan , Jianfa Wang , Q. Daniel Wang , Yang Yang

The edge-on galaxy NGC 4565 has been observed in the 12CO(J=1-0)-line emission using the Nobeyama 45-m telescope with an angular resolution of 15". We obtained a scan along the major axis for +/-5' (+/- 15 kpc) about the galactic center,…

天体物理学 · 物理学 2007-05-23 Y. Sofue , N. Nakai

We have obtained high signal-to-noise spectra along the major axes of 28 S0 galaxies in order to search for the presence of disk stars on retrograde orbits. Full line-of-sight velocity distributions were extracted from the data, and the…

天体物理学 · 物理学 2015-06-24 Konrad Kuijken , David Fisher , Michael R. Merrifield

We present new mm interferometric and optical integral-field unit (IFU) observations and construct a sample of 12 E and S0 galaxies with molecular gas which have both CO and optical maps. The galaxies contain 2 x 10^7 to 5 x 10^9 M\odot of…

宇宙学与河外天体物理 · 物理学 2015-05-19 Alison F. Crocker , Martin Bureau , Lisa M. Young , Francoise Combes

We present IRAM 30m observations of molecular lines of CO and its isotopologues from the massive spiral galaxy NGC 5908 selected from the CGM-MASS sample. $^{12}$CO $J=1-0$, $^{12}$CO $J=2-1$, and $^{13}$CO $J=1-0$ lines have been detected…

星系天体物理 · 物理学 2019-05-29 Jiang-Tao Li , Ping Zhou , Xuejian Jiang , Joel N. Bregman , Yu Gao

We present high-resolution (0.94" $\approx$ 55 pc) ALMA CO(2-1) and 13CO(2-1) observations of the highly inclined (i~87.5 deg) galaxy NGC 4565 covering out to galactocentric radius Rgal > $\pm$ 17 kpc. The combination of sensitivity and…

Observations of 12CO J=1-0 and HCN J=1-0 emission from NGC 5194 (M51) made with the 50~meter Large Millimeter Telescope and the SEQUOIA focal plane array are presented. Using the HCN to CO ratio, we examine the dense gas mass fraction over…

The edge-on Sc galaxy NGC 5907 has been observed in the 12CO(1-0)-line emission using the Nobeyama 45-m telescope. The radial density distribution between 2 and 13 kpc is well represented by a superposition of an exponential-law disk of…

天体物理学 · 物理学 2007-05-23 Yoshiaki SOFUE
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