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相关论文: Arp 58 and Arp 68: two M 51- type systems

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We present ALMA observations of a merging system at z ~ 4.57, observed as a part of the ALMA Large Program to INvestigate [CII] at Early times (ALPINE) survey. Combining ALMA [CII] 158 micron and far-infrared continuum data with…

This paper presents a detailed analysis of two-armed spiral structure in a sample of galax- ies from the Spitzer Infrared Nearby Galaxies Survey (SINGS), with particular focus on the relationships between the properties of the spiral…

星系天体物理 · 物理学 2015-06-23 S. Kendall , C. Clarke , R. C. Kennicutt

We investigate dynamical states of grand-design spiral arms in three local galaxies: M51, NGC3627 and NGC628. Based on linear perturbation analysis considering multiple components in the galaxies, we compute instability parameters of the…

星系天体物理 · 物理学 2021-06-30 Shigeki Inoue , Toshinobu Takagi , Atsushi Miyazaki , Erin Mentuch Cooper , Fumi Egusa , Hidenobu Yajima

We investigate the cold and warm gas content, kinematics, and spatial distribution of six local massive elliptical galaxies to probe the origin of the multiphase gas in their atmospheres. We report new observations, including SOFIA [CII],…

星系天体物理 · 物理学 2022-04-13 P. Temi , M. Gaspari , F. Brighenti , N. Werner , R. Grossova , M. Gitti , M. Sun , A. Amblard , A. Simionescu

We discuss the integrated kinematic parameters of 20 M51-type binary galaxies. A comparison of the orbital masses of the galaxies with the sum of the individual masses suggests that moderately massive dark halos surround bright spiral…

天体物理学 · 物理学 2009-11-07 V. P. Reshetnikov , S. A. Klimanov

We show the variations of the CO J=2-1/1-0 line ratio (R21) across the barred spiral galaxy M83, using the 46 pc resolution data from ALMA. The R21 map clearly evidences the systematic large-scale variations as a function of galactic…

星系天体物理 · 物理学 2025-05-15 Jin Koda , Fumi Egusa , Akihiko Hirota , Amanda M Lee , Tsuyoshi Sawada , Fumiya Maeda

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 revisit the orbital history of the Triangulum galaxy (M33) around the Andromeda galaxy (M31) in view of the recent Gaia Data Release 2 proper motion measurements for both Local Group galaxies. Earlier studies consider highly idealised…

星系天体物理 · 物理学 2020-02-05 Thor Tepper-García , Joss Bland-Hawthorn , Di Li

We use a data set of nearby galaxies drawn from the HERACLES, ATLAS3D, and COLD GASS surveys to study variations in molecular gas depletion time (Tdep) in galaxy structures such as bulges, grand-design spiral arms, bars and rings. Molecular…

星系天体物理 · 物理学 2015-06-23 Mei-Ling Huang , Guinevere Kauffmann

We study a peculiar galaxy NGC 90, a pair member of interacting system Arp 65 (NGC 90/93), using the long-slit spectral observations carried out at the Russian 6m telescope BTA and the available SDSS photometric data. This galaxy…

星系天体物理 · 物理学 2020-08-12 Anatoly V. Zasov , Anna S. Saburova , Oleg V. Egorov , Alexey V. Moiseev

As the nearest large spiral galaxy, M31 provides a unique opportunity to learn about the structure and evolutionary history of this galaxy type in great detail. Among the many observing programs aimed at M31 are microlensing studies, which…

We present a kinematic catalogue for 21 M51-type galaxies. It consists of radial velocity distributions observed with long slit spectroscopy along different position angles, for both the main and satellite components. We detect deviations…

星系天体物理 · 物理学 2016-11-09 G. Gunthardt , R. J. Díaz , M. P. Aguero

Using the B-I color index in the radial photometry of M51, applied to defined azimuthal sectors, we reveals asymmetries in the shape of the density pattern of the galactic arms. The anomalous shape is present only in the side close to the…

天体物理学 · 物理学 2007-05-23 F. Natali , L. Di Fino , G. Natali

The density wave theory predicted some physical offsets among different tracers of star formation. To test this prediction, here we compiled data on 40 galaxies searched observationally for a physical offset between spiral arm tracers, and…

星系天体物理 · 物理学 2019-11-21 Jacques P Vallee

Spiral arms are common features in low-redshift disc galaxies, and are prominent sites of star-formation and dust obscuration. However, spiral structure can take many forms: from galaxies displaying two strong `grand design' arms, to those…

We present a detailed and uniform study of oxygen abundance from two different oxygen lines at 6158$\AA$ and 6300$\AA$ in a large sample of solar-type stars. The results are used to check the behaviour of these spectral lines as oxygen…

太阳与恒星天体物理 · 物理学 2015-04-15 S. Bertran de Lis , E. Delgado Mena , V. Zh. Adibekyan , N. C. Santos , S. G. Sousa

We present a spatially-resolved analysis of ionized and molecular gas in a nearby Seyfert 2 galaxy NGC 5728, using the VLT/MUSE and ALMA data. We find ionized gas outflows out to ~kpc scales, which encounter the star formation ring at 1 kpc…

星系天体物理 · 物理学 2019-09-04 Jaejin Shin , Jong-Hak Woo , Aeree Chung , Junhyun Baek , Kyuhyoun Cho , Daeun Kang , Hyun-Jin Bae

We describe the structure and composition of six major stellar streams in a population of 20 574 local stars in the New Hipparcos Reduction with known radial velocities. We find that, once fast moving stars are excluded, almost all stars…

综合物理 · 物理学 2010-01-15 Charles Francis , Erik Anderson

We present the results of optical long-slit spectral observations of interacting system Arp305 carried out at the 6m telescope BTA at the SAO RAS: the radial variation of gas kinematics and oxygen abundance. This study continues the series…

星系天体物理 · 物理学 2018-06-06 Anatoly V. Zasov , Anna S. Saburova , Oleg V. Egorov , Viktor L. Afanasiev