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相关论文: The hidden HI-massive LIRG HIZOA J0836-43: Inside-…

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HIZOA J0836-43 is the most HI-massive (M_HI = 7.5x10^10 Msun) galaxy detected in the HIPASS volume and lies optically hidden behind the Milky Way. Markedly different from other extreme HI disks in the local universe, it is a luminous…

宇宙学与河外天体物理 · 物理学 2015-05-20 M. E. Cluver , T. H. Jarrett , R. C. Kraan-Korteweg , B. S. Koribalski , P. N. Appleton , J. Melbourne , B. Emonts , P. A. Woudt

HIZOA J0836-43is one of the most HI-massive galaxies in the local (z<0.1) Universe. Not only are such galaxies extremely rare, but this "coelacanth" galaxy exhibits characteristics -- in particular its active, inside-out stellar…

宇宙学与河外天体物理 · 物理学 2015-06-03 Renee C. Kraan-Korteweg , Michelle E. Cluver

Little is known about the properties of extremely massive HI-galaxies. They are extremely scarce and are - according to hierarchical structure formation - only forming now (z < 1). The forthcoming deep HI SKA Pathfinders surveys will…

宇宙学与河外天体物理 · 物理学 2009-09-16 Renee C. Kraan-Korteweg , Michelle Cluver , Tom H. Jarrett , Patrick A. Woudt

We report the discovery of a very HI-massive disk galaxy, HIZOA J0836-43, at a velocity of v_hel = 10689 km/s, corresponding to a distance of 148 Mpc (assuming H_0=75 km/s/Mpc). It was found during the course of a systematic HI survey of…

A first analysis of a deep blind HI survey covering the southern Zone of Avoidance plus an extension towards the north (196 < l < 52 deg) obtained with the Multibeam receiver at the 64m Parkes telescope reveals slightly over a thousand…

天体物理学 · 物理学 2007-05-23 R. C. Kraan-Korteweg , L. Staveley-Smith , J. Donley , P. A. Henning , ;

We report deep ALMA observations complemented with associated HST imaging for a luminous (m_uv=25) galaxy, `Himiko', at a redshift z=6.595. The galaxy is remarkable for its high star formation rate, 100 Mo/yr, securely estimated from our…

Aims: To explore the infrared and radio properties of one of the closest Galactic starburst regions. Methods: Images obtained with the Herschel Space Observatory at wavelengths of 70, 160, 250, 350, and 500 microns using the PACS and SPIRE…

We report the discovery of a 20-kpc-sized H{\alpha} emission in SDSS J083803.68+540642.0, a ringed dwarf galaxy (M$_V$ = -17.89 mag) hosting an accreting intermediate-mass black hole at z=0.02957. Analysis of the HST images indicates that…

星系天体物理 · 物理学 2017-03-15 Wen-Juan Liu , Lei Qian , Xiao-Bo Dong , Ning Jiang , Paulina Lira , Zheng Cai , Feige Wang , Jinyi Yang , Ting Xiao , Minjin Kim

Chemical abundances in the Leo ring, the largest HI cloud in the local Universe, have recently been determined to be close or above solar, incompatible with a previously claimed primordial origin of the ring. The gas, pre-enriched in a…

星系天体物理 · 物理学 2021-07-21 Edvige Corbelli , Filippo Mannucci , David Thilker , Giovanni Cresci , Giacomo Venturi

Based on a new HI survey using the Five-hundred-meter Aperture Spherical radio Telescope (FAST), combined with the Pan-STARRS1 images, we identified an isolated HI cloud without any optical counterpart, named FAST J0139+4328. The newly…

宇宙学与河外天体物理 · 物理学 2023-03-01 Jin-Long Xu , Ming Zhu , Naiping Yu , Chuan-Peng Zhang , Xiao-Lan Liu , Mei Ai , Peng Jiang

We present a first look at the local LIRG, IRAS04296+2923. This barred spiral, overlooked because of its location in the Galactic plane, is among the half dozen closest LIRGs. More IR-luminous than either M82 or the Antennae, it may be the…

星系天体物理 · 物理学 2015-05-19 David S. Meier , Jean L. Turner , Sara C. Beck , Varoujan Gorjian , Chao-Wei Tsai , Schuyler D. Van Dyk

We present detailed images of diffuse UV intergalactic light (IGL), situated in a 60kpc halo that surrounds the radio galaxy MRC 1138-262 at z=2. We discuss the nature of the IGL and rule out faint cluster galaxies, nebular continuum…

天体物理学 · 物理学 2009-11-13 N. A. Hatch , R. A. Overzier , H. J. A. Röttgering , J. D. Kurk , G. K. Miley

We present the discovery of 2MASS J05241392-0336543 (hereafter J0524-0336), a very metal-poor ([Fe/H]=-2.43 +- 0.16), highly r-process-enhanced ([Eu/Fe]= +1.34 +- 0.10) Milky Way halo field red giant star, with an ultra high Li abundance of…

An analysis of data from the Spitzer Space Telescope, Hubble Space Telescope, Chandra X-ray Observatory, and AKARI Infrared Astronomy Satellite is presented for the z=0.036 merging galaxy system II Zw 096 (CGCG 448-020). Because II Zw 096…

We present a detailed analysis of J154506, a strongly lensed submillimeter galaxy behind the Lupus-I molecular cloud, and characterisation of its physical properties using a combination of new and archival data, including VLT/MUSE and FORS2…

Though S0 galaxies are usually thought to be `red and dead', they demonstrate often star formation organized in ring structures. We try to clarify the nature of this phenomenon and its difference from star formation in spiral galaxies. The…

星系天体物理 · 物理学 2020-07-01 Olga Sil'chenko , Alexei Moiseev

The filament IRDC G035.39--00.33 in the W48 molecular complex is one of the darkest infrared clouds observed by \textit{Spitzer}. It has been observed by the PACS (70 and 160\,$\micron$) and SPIRE (250, 350, and 500\,$\micron$) cameras of…

The nearby galaxy HIZSS003 was recently discovered during a blind HI survey of the zone of avoidance (Henning et al. 2000). Follow up VLA as well as optical and near-IR imaging and spectroscopy (Massey et al. 2003; Silva et al. 2005)…

天体物理学 · 物理学 2009-11-10 Ayesha Begum , Jayaram N. Chengalur , I. D. Karachentsev , M. E. Sharina

The known host galaxies of short-hard gamma-ray bursts (GRBs) to date are characterized by low to moderate star-formation rates and a broad range of stellar masses. In this paper, we positionally associate the recent unambiguously…

高能天体物理现象 · 物理学 2015-06-03 Daniel A. Perley , M. Modjaz , A. N. Morgan , S. B. Cenko , J. S. Bloom , N. R. Butler , A. V. Filippenko , A. A. Miller

We carry out sensitive searches for the CO J=1-0 and J=2-1 lines in the giant extragalactic HI ring in Leo to investigate the star formation process within environments where gas metallicities are close to solar but physical conditions are…

星系天体物理 · 物理学 2023-03-15 Edvige Corbelli , David Thilker , Filippo Mannucci , Giovanni Cresci
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