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Related papers: Outflow from Outer-arm Starburst in a Grazing Coll…

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We present ALMA Cycle-0 observations of the CO (6-5) line emission (rest-frame frequency = 691.473 GHz) and of the 435$\mu m$ dust continuum emission in the nuclear region of NGC 34, a local luminous infrared galaxy (LIRG) at a distance of…

We present a comprehensive physical and chemical study of the fragmentation and star formation activity towards the massive clump AGAL G338.9188+0.5494 harbouring the extended green object EGO 338.92+0.55(b). The presence of an EGO embedded…

Astrophysics of Galaxies · Physics 2023-09-20 M. E. Ortega , N. C. Martinez , S. Paron , A. Marinelli , N. L. Isequilla

The physical properties of galactic molecular outflows are important as they could constrain outflow formation mechanisms. We study the properties of the southwest (SW) outflow streamer including gas kinematics, optical depth, dense gas…

The gas content of galaxies is a key factor for their growth, starting from star formation and black hole accretion to galaxy mergers. Thus, characterising its properties via observations of tracers like the CO emission line is of big…

Astrophysics of Galaxies · Physics 2020-02-26 Judit Fogasy , Kirsten K. Knudsen , Guillaume Drouart , Claudia del P. Lagos , Lulu Fan

Radio continuum, Spitzer infrared, optical and XMM-Newton X-ray and UVM2 observations are used to study large-scale shock fronts, young star complexes, and the galactic nuclei in the interacting galaxies NGC 2207/IC 2163. There are two…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-27 Michele Kaufman , Dirk Grupe , Debra M. Elmegreen , Bruce G. Elmegreen , Curtis Struck , Elias Brinks

We present our high-resolution ($0^{\prime\prime}.15\times0^{\prime\prime}.13$, $\sim$34 pc) observations of the CO(6-5) line emission, which probes the warm and dense molecular gas, and the 434 $\mu$m dust continuum emission in the nuclear…

High-mass stars, with their powerful winds and intense radiation fields, are fundamental in regulating galactic dynamics and evolution; however, despite their great relevance, the mechanisms involved in their formation are still not fully…

Astrophysics of Galaxies · Physics 2026-03-19 E. Cohen Arazi , M. E. Ortega , S. Paron , P. F. Velázquez , A. Rodríguez-González , E. Alquicira

We report ALMA observations of CO(3-2) emission in the Seyfert 2 double-barred galaxy NGC1433, at the unprecedented spatial resolution of 0.5"=24 pc. Our aim is to probe AGN feeding and feedback phenomena through the morphology and dynamics…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-17 F. Combes , S. Garcia-Burillo , V. Casasola , L. K. Hunt , M. Krips , A. J. Baker , F. Boone , A. Eckart , I. Marquez , R. Neri , E. Schinnerer , L. J. Tacconi

We present new ALMA observations of a starburst galaxy at cosmic noon hosting a radio-loud active galactic nucleus: PKS 0529-549 at $z=2.57$. To investigate the conditions of its cold interstellar medium, we use ALMA observations which…

We present a new 12CO(J=1-0)-line survey of the Andromeda galaxy, M31, covering the bright disk with the highest resolution to date (85 pc along the major axis), observed On-the-Fly (in italics) with the IRAM 30-m telescope. We discuss the…

ALMA observations in the CO 1 - 0 line of the interacting galaxies IC 2163 and NGC 2207 at 2" x 1.5" resolution reveal how the encounter drives gas to pile up in narrow, ~ 1 kpc wide, "eyelids" in IC 2163. IC 2163 and NGC 2207 are involved…

We investigate the ionized gas excitation and kinematics in the inner $4.3 \times 6.2$ kpc$^{2}$ of the merger radio galaxy 4C +29.30. Using optical integral field spectroscopy with the Gemini North Telescope, we present flux distributions,…

Large-scale outflows are believed to be an important mechanism in the evolution of galaxies. We can determine the impact of these outflows by studying either current galaxy outflows and their effect in the galaxy or by studying the effect…

Astrophysics of Galaxies · Physics 2023-01-11 J. Scholtz , R. Maiolino , G. C. Jones , S. Carniani

Massive molecular outflows erupting from high-mass young stellar objects provide important clues to understanding the mechanism of high-mass star formation. Based on new CO J=3-2 and J=1-0 observations using the Atacama Submillimeter…

Young massive clusters play an important role in the evolution of their host galaxies, and feedback from the high-mass stars in these clusters can have profound effects on the surrounding interstellar medium. The nuclear starburst in the…

ALMA observations of the Galactic center with spatial resolution $2.61"\times0.97"$ resulted in the detection of 11 SiO (5-4) clumps of molecular gas within 0.6pc (15$"$) of Sgr A*, interior to the 2-pc circumnuclear molecular ring. The…

Astrophysics of Galaxies · Physics 2015-06-15 F. Yusef-Zadeh , M. Royster , M. Wardle , R. Arendt , H. Bushouse , D. C. Lis , M. W. Pound , D. A. Roberts , B. Whitney , A. Wootten

Arcsecond-resolution X-ray imaging of the nucleus of the nearby starburst galaxy NGC 253 with Chandra reveals a well-collimated, strongly limb-brightened, kiloparsec-scale conical outflow from the central starburst region. The outflow is…

Astrophysics · Physics 2009-10-31 David K. Strickland , Timothy M. Heckman , Kimberly A. Weaver , Michael Dahlem

This paper reports on the detection of a likely explosive outflow in the high-mass star-forming complex G34.26+0.15, adding to the small number (six) of explosive outflows detected so far. ALMA CO(2-1) and SiO(5-4) archival observations…

Solar and Stellar Astrophysics · Physics 2025-04-23 Namitha Issac , Xing Lu , Tie Liu , Luis A Zapata , Hong-Li Liu , Anandmayee Tej , Yan-Kun Zhang , Wenyu Jiao , Suinan Zhang

We present Atacama Large Millimeter/Submillimeter Array (ALMA) CO (1-0) and CO (3-2) observations of SDSS J135646.10+102609.0, an obscured quasar and ultra-luminous infrared galaxy (ULIRG) with two merging nuclei and a known 20-kpc-scale…

Astrophysics of Galaxies · Physics 2015-06-22 Ai-Lei Sun , Jenny E. Greene , Nadia L. Zakamska , Nicole P. H. Nesvadba

The red hypergiant VY CMa is famous for its very visible record of high mass loss events. Recent CO observations with ALMA revealed three previously unknown large scale outflows (Paper I). In this paper we use the CO maps to investigate the…

Solar and Stellar Astrophysics · Physics 2024-01-29 Roberta M. Humphreys , A. M. S. Richards , Kris Davidson , A. P. Singh , L. Decin , L. M. Ziurys