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相关论文: BVR photometry of the resolved dwarf galaxy Ho IX

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We have carried out CCD photometry in the Cousins B and R bands of 21 dwarf galaxies in and around the M101 group. Eleven are members and suspected members of the group and ten are field galaxies in the projected vicinity of the group. We…

天体物理学 · 物理学 2009-10-31 T. Bremnes , B. Binggeli , P. Prugniel

We have surveyed a complete extent of Leo A - an apparently isolated gas-rich low-mass dwarf irregular galaxy in the Local Group. The $B$, $V$, and $I$ passband CCD images (typical seeing $\sim$0.8") were obtained with Subaru Telescope…

星系天体物理 · 物理学 2014-10-10 R. Stonkutė , N. Arimoto , T. Hasegawa , D. Narbutis , N. Tamura , V. Vansevičius

CCD - photometry is presented for 20 dIrr galaxies situated in the nearby complexes CenA/M83, and CVnI as well as in the general field of the Local Volume. We present integrated magnitudes of the galaxies in B,V,I - bands and also surface…

宇宙学与河外天体物理 · 物理学 2015-05-13 L. Makarova , I. Karachentsev , L. Rizzi , R. B. Tully , G. Korotkova

Deep images taken with the Wide Field Channel of the Advanced Camera for Surveys on board the Hubble Space Telescope provide the basis for study the resolved stellar population of the M81 companion dwarf irregular galaxy Holmberg IX. Based…

天体物理学 · 物理学 2009-11-13 E. Sabbi , J. S. Gallagher , L. J. Smith , D. F. de Mello , M. Mountain

Using the Canada-France-Hawaii Telescope we have obtained deep high-resolution CCD images in V and I of a 28'x28' field in the outer disk of M 31 at ~ 116' from the center along the major axis to the south-west, and covering a range of…

天体物理学 · 物理学 2009-11-06 Jean-Charles Cuillandre , James Lequeux , Ronald J. Allen , Yannick Mellier , Emmanuel Bertin

We present observations and analysis of nine dwarf irregular galaxies (dIs) in the M81 Group taken with the Advanced Camera for Surveys aboard the Hubble Space Telescope. The nine galaxy sample (the Garland, M81 Dwarf A, DDO 53, Ho IX, Ho…

We present images and a color-magnitude diagram for And V, a new dwarf spheroidal companion to M31 that was found using a digital filtering technique applied to 1550 square degrees of the second Palomar Sky Survey. And V resolves into stars…

天体物理学 · 物理学 2009-10-30 Taft E. Armandroff , James E. Davies , George H. Jacoby

We report the discovery of a new dwarf spheroidal satellite of M31, Andromeda IX, based on resolved stellar photometry from the Sloan Digital Sky Survey (SDSS). Using both SDSS and public archival data we have estimated its distance and…

We present WIYN observations of the recently discovered And IX dwarf spheroidal (dSph) satellite galaxy of M 31. Our data, obtained at a natural seeing of 0.5'' and just reaching the horizontal branch level, confirm And IX as a dSph galaxy…

天体物理学 · 物理学 2011-08-23 D. Harbeck , J. Gallagher , E. K. Grebel , A. Koch , D. Zucker

We present our B, V, Rc, and Ic observations of a 3.6' x 3' field centered on the host galaxy of GRB000926 (RA(2000.0)=17h04m11s, DEC(2000.0)=+51d47'9.8''). The observations were carried out on the 6-m Special Astrophysical Observatory…

天体物理学 · 物理学 2009-11-10 T. A. Fatkhullin , A. A. Vasil'ev , V. P. Reshetnikov

We examine the stellar content of 10 dwarf irregular galaxies of which broad-band CCD photometry was published in Hopp & Schulte-Ladbeck (1995). We also present Halpha images for several of these galaxies. The galaxies in the sample are…

天体物理学 · 物理学 2009-10-30 Regina E. Schulte-Ladbeck , Ulrich Hopp

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

This paper is the first in a series presenting CCD multicolor photometry for 145 HII regions, selected from 369 candidate regions from Boulesteix et al. (1974), in the nearby spiral galaxy M33. The observations, which covered the whole area…

天体物理学 · 物理学 2009-11-07 Linhua Jiang , Jun Ma , Xu Zhou , Jiansheng Chen , Hong Wu , Zhaoji Jiang , Suijian Xue , Jin Zhu

We present the results from a search for HI emission from a sample of newly discovered dwarf galaxies in the M81 group. HI is detected in three galaxies, all of which are classified as BCDs. The HI masses of these galaxies are ~ 10^6 M_sun,…

宇宙学与河外天体物理 · 物理学 2014-09-04 Sambit Roychowdhury , Jayaram N. Chengalur , Kristin Chiboucas , Igor D. Karachentsev , R. Brent Tully , Serafim S. Kaisin

We present deep BVRI band images and HI line observations of the nearby, low surface brightness galaxy ESO215-G?009 which were obtained with the ANU 2.3-m Telescope and the Australia Telescope Compact Array, respectively. ESO215-G?009 was…

天体物理学 · 物理学 2009-11-10 Bradley E. Warren , Helmut Jerjen , Baerbel S. Koribalski

We have carried out surface photometry of four bright known members and a number of new possible LSB companions of the IC 65 (LGG 16) group of galaxies. The purpose of the present study is twofold: (a) a search for new LSB dwarf members and…

天体物理学 · 物理学 2007-05-23 J. Vennik , U. Hopp

We report the discovery of a new dwarf galaxy, Andromeda XXVIII, using data from the recently-released SDSS DR8. The galaxy is a likely satellite of Andromeda, and, at a separation of $365^{+17}_{-1}$ kpc, would be one of the most distant…

星系天体物理 · 物理学 2015-05-30 Colin T. Slater , Eric F. Bell , Nicolas F. Martin

We present B-, V-, and I-band images, as well as an H alpha image, of And VI. This is the second newly identified dwarf spheroidal (dSph) companion to M31 found using a digital filtering technique applied to the second Palomar Sky Survey…

天体物理学 · 物理学 2009-10-31 Taft E. Armandroff , George H. Jacoby , James E. Davies

Long-slit spectroscopy has been obtained for a sample of 22 blue dwarf galaxies selected in the direction of the Virgo Cluster as part of a larger sample of Virgo blue dwarf galaxies for which deep Halpha imaging has been collected. Most of…

天体物理学 · 物理学 2009-11-07 J. M. Vilchez , J. Iglesias-Paramo

We present optical observations of an ultraluminous X-ray source (ULX) in Holmberg IX, a dwarf galaxy near M81. The ULX has an average X-ray luminosity of some 10^{40} erg/s. It is located in a huge (400pc x 300pc) ionized nebula being much…

天体物理学 · 物理学 2009-11-11 Fabien Grise , Manfred W. Pakull , Christian Motch
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