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相关论文: A search for HI in some peculiar faint dwarf galax…

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The goal of this study is to measure parameters of the integrated HI emission for twenty-two dwarf galaxies with oxygen abundance 12+log(O/H) in the range of 7.42 to 7.65, which are representatives of the eXtremely Metal-Deficient (XMD)…

天体物理学 · 物理学 2009-11-13 S. A. Pustilnik , J. -M. Martin

We present large field HI-line emission maps obtained with the single-dish Green Bank Telescope centered on the dwarf irregular galaxies Sextans A, NGC 2366, and WLM. We do not detect the extended skirts of emission associated with the…

宇宙学与河外天体物理 · 物理学 2015-05-30 Deidre A. Hunter , Fakhri Zahedy , Emily C. Bowsher , Eric M. Wilcots , Amanda A. Kepley , Veronika Gaal

We report a $\approx 400$-hour Giant Metrewave Radio Telescope (GMRT) search for HI 21 cm emission from star-forming galaxies at $z = 1.18-1.39$ in seven fields of the DEEP2 Galaxy Survey. Including data from an earlier 60-hour GMRT…

星系天体物理 · 物理学 2021-06-09 Aditya Chowdhury , Nissim Kanekar , Barnali Das , K. S. Dwarakanath , Shiv Sethi

Previous searches for HI in our Galaxy's dwarf spheroidal companions have not been complete enough to settle the question of whether or not these galaxies have HI, especially in their outer parts. We present VLA observations of three dwarf…

天体物理学 · 物理学 2009-10-31 L. M. Young

We describe the design, data analysis, and basic results of the Giant Metrewave Radio Telescope Cold-HI AT $z\approx1$ (GMRT-CAT$z$1) survey, a 510-hour upgraded GMRT HI 21 cm emission survey of galaxies at $z=0.74-1.45$ in the DEEP2 survey…

星系天体物理 · 物理学 2022-10-04 Aditya Chowdhury , Nissim Kanekar , Jayaram N. Chengalur

We present a ground-based optical spectroscopic and HST U, V, I photometric study of the blue compact dwarf (BCD) galaxy Pox 186. It is found that the emission of the low-surface brightness (LSB) component in Pox 186 at radii < 3'' (< 270…

天体物理学 · 物理学 2009-11-10 N. G. Guseva , P. Papaderos , Y. I. Izotov , K. G. Noeske , K. J. Fricke

We present new HI data of the dwarf galaxy KK 69, obtained with the Giant Metrewave Radio Telescope (GMRT) with a signal-to-noise ratio that almost double previous observations. We carried out a Gaussian spectral decomposition and stacking…

星系天体物理 · 物理学 2020-07-15 J. Saponara , B. S. Koribalski , N. N. Patra , P. Benaglia

Previous searches for atomic gas in our Galaxy's dwarf spheroidal companions have not been complete enough to settle the question of whether or not these galaxies have HI, especially in their outer parts. We present new observations of the…

天体物理学 · 物理学 2009-10-31 L. M. Young

Sensitive 21cm HI line observations were performed for 23 dwarf members and possible members of the nearby M81 group of galaxies, including five objects of a clustering of extremely low-surface brightness objects of unknown nature. With the…

天体物理学 · 物理学 2007-05-23 W. van Driel , R. C. Kraan-Korteweg , B. Binggeli , W. K. Huchtmeier

We compare the gas distribution, kinematics and the current star formation in a sample of 10 very faint (-13.37 < M_B < -9.55) dwarf galaxies. For 5 of these galaxies we present fresh, high sensitivity, GMRT HI 21cm observations. For all…

天体物理学 · 物理学 2009-11-13 Ayesha Begum , Jayaram. N. Chengalur , I. D. Karachentsev , S. S. Kaisin , M. E. Sharina

We model the observed vertical distribution of the neutral hydrogen (HI) in the faint (M_B ~ -13.7 mag) edge-on dwarf irregular galaxy KK250. Our model assumes that the galaxy consists of axi-symmetric, co-planar gas and stellar discs in…

星系天体物理 · 物理学 2014-11-18 Narendra Nath Patra , Arunima Banerjee , Jayaram N. Chengalur , Ayesha Begum

We present results of deep, high velocity resolution ($\sim$1.6 kms$^{-1}$) Giant Meterwave Radio Telescope (GMRT) HI 21 cm-line observations of a sample of extremely faint (M$_B>-$12.5) dwarf irregular galaxies. Unlike previous studies, we…

天体物理学 · 物理学 2007-05-23 Ayesha Begum , Jayaram N. Chengalur

We identify 814 discrete HI clouds in 40 dwarf irregular galaxies from the LITTLE THINGS survey using an automated cloud-finding algorithm. The cloud masses range from ~10^3 to 10^7 Msolar, have a surface density averaged over all of the…

星系天体物理 · 物理学 2019-06-05 Deidre A. Hunter , Bruce G. Elmegreen , Clara L. Berger

HI observations of the nearby blue compact dwarf galaxy IC 10 obtained with the Dominion Radio Astrophysical Observatory synthesis telescope (DRAO), for a total integration of $\sim$1000 hours, are presented. We confirm the NW faint 21 cm…

星系天体物理 · 物理学 2020-01-08 Brenda Namumba , Claude Carignan , Tyler Foster , Nathan Deg

We have used the VLA to image the HI 21-cm line emission in the edge-on Sd galaxy IC2233 and the blue compact dwarf NGC2537. We also present new optical B,R, and H alpha imaging of IC2233 obtained with the WIYN telescope. Despite evidence…

天体物理学 · 物理学 2008-11-26 Lynn D. Matthews , Juan M. Uson

We present and discuss the results of the Giant Metrewave Radio Telescope (GMRT) HI 21-cm line mapping for five isolated low-mass (M_bary ~(2--8)*10^7 Mo) eXtremely Metal Poor (XMP) dwarfs [12+log(O/H)=7.13-7.28], selected from the Nearby…

星系天体物理 · 物理学 2024-08-05 Sushma Kurapati , Simon A. Pustilnik , Evgeniya S. Egorova

We report a deep search for HI 21cm emission from the $z= 0.00632$ sub-DLA toward PG1216+069 with the Giant Metrewave Radio Telescope. No emission was detected and our $5\sigma$ upper limit on the mass of any associated galaxy is $M_{\rm…

天体物理学 · 物理学 2009-11-10 Nissim Kanekar , Jayaram N. Chengalur

We report on the HI content of an isolated, compact group of 6 dwarf galaxies at a distance of 145 Mpc. The distribution and kinematics of the HI, including multiple gaseous bridges, indicate the group is a gravitationally bound system. The…

We present HI observations of four giant low surface brightness (GLSB) galaxies UGC 1378, UGC 1922, UGC 4422 and UM 163 using the Giant Meterwave Radio Telescope (GMRT). We include HI results on UGC 2936, UGC 6614 and Malin 2 from…

星系天体物理 · 物理学 2016-10-12 Alka Mishra , N. G. Kantharia , M. Das , A. Omar , D. C. Srivastava

We present Giant Metrewave Radio Telescope 21-cm HI observations towards a sample of compact radio sources behind galaxy groups, to search for cool HI. The results -- from high dynamic range spectra for 8 lines-of-sight through 7 galaxy…

天体物理学 · 物理学 2014-10-13 D. A. Green , M. S. Clemens , P. Alexander , H. Cullen , B. Nikolic
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