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Related papers: M31 and Local Group QSO's

200 papers

We present spectroscopy of nine planetary nebulae (PNe) in the outskirts of M31, all but one obtained with the 10.4m GTC telescope. These sources extend our previous study of the oxygen abundance gradient of M31 to galactocentric radii as…

Astrophysics of Galaxies · Physics 2015-07-15 R. L. M. Corradi , K. B. Kwitter , B. Balick , R. B. C. Henry , K. Hensley

We report the discovery of a high redshift, narrow emission-line galaxy identified in the optical follow-up of deep ROSAT fields. The object has a redshift of z=2.35 and its narrow emission lines together with its high optical and X-ray…

Astrophysics · Physics 2007-05-23 O. Almaini , B. J. Boyle , R. E. Griffiths , T. Shanks , G. C. Stewart , I. Georgantopoulos

NGC 613 (AM 0132-294) is a multi armed spiral with an active nucleus. Radio emission is aligned along the narrow inner bar of the spiral and appears to include inner and outer pairs of radio sources which define a line of ejection from this…

Astrophysics · Physics 2007-05-23 H. Arp

We report a survey for molecular gas in 3C radio galaxies at redshifts z < 0.031. Four of the twenty-three galaxies observed were detected with molecular gas masses in the range 10^7--10^9 Msun. The remainder had typical upper limits in…

Astrophysics · Physics 2007-05-23 Jeremy Lim , Stephane Leon , Francoise Combes , Dinh-V-Trung

Massive, quiescent galaxies are already observed at redshift $z\sim4$, i.e. $\sim$1.5 Gyr after the Big Bang. Current models predict them to be formed via massive, gas-rich mergers at $z>6$. Recent ALMA observations of the cool gas and dust…

Photometry is presented in R, J, H, K of the z=2.37 QSO 0820+296 and its environment. Colours and magnitudes of most of the objects within 50 arcsec of the QSO suggest they are a group of galaxies at the QSO redshift with a young stellar…

Astrophysics · Physics 2009-10-30 J. B. Hutchings , S. G. Neff

We searched the Sloan Digital Sky Survey for outer halo globular clusters (GCs) around M31. Our search of non-stellar objects, within the limits 0.3 < (g-i)o < 1.5 and 14.0 < ro < 19.0 concentrated in some remote areas of the extended halo,…

Astrophysics of Galaxies · Physics 2015-06-12 Graziella di Tullio Zinn , Robert Zinn

Deep UBRI images of a 15'x15' field in the M31 galaxy's outer spheroid obtained with the KPNO 4-m telescope, and Keck 10-m telescope+LRIS I-band images, are used to isolate candidate red giant branch stars located at R=19 kpc (projected)…

Astrophysics · Physics 2009-10-30 David B. Reitzel , Puragra Guhathakurta , Andrew Gould

Some recent work on radio source fields at z~0.7 and z~4 is discussed. At z~0.7 we find that radio-loud quasars are typically found in moderately rich environments independent of radio luminosity, consistent with previous results at z~0.5.…

Astrophysics · Physics 2007-05-23 M. Lacy

(Abridged) We report the discovery of an X-ray group of galaxies located at a high redshift of z=1.61 in the Chandra Deep Field South. The group is first identified as an extended X-ray source. We use a wealth of deep multi-wavelength data…

We report the first results from deep ACS imaging of ten classical globular clusters in the far outer regions (15 < R_p < 100 kpc) of M31. Eight of the clusters, including two of the most remote M31 globular clusters presently known, are…

We present Hubble Space Telescope/WFPC2 images of sixteen dwarf galaxies as part of our snapshot survey of nearby galaxy candidates. We derive their distances from the luminosity of the tip of the red giant branch stars with a typical…

This study on the Coma cluster suggests that there are deviations from a completely random galaxy orientation on small scales. Since we found a significant coincidence of hot-gas features identified in the latest X-ray observations of Coma…

Astrophysics · Physics 2009-11-07 M. G. Kitzbichler , W. Saurer

We present results of a CO(1-0) line survey in a complete sample of 12 low redshift (Z < 0.1), optically bright QSOs (PG QSOs with M_B < -23 mag). Six new CO detections are reported here at levels exceeding I_CO ~2 Jy km/s. Combined with…

Astrophysics · Physics 2009-11-07 N. Z. Scoville , D. T. Frayer , E. Schinnerer , M. Christopher

We analyse new deep g and i-band imaging with the CFHT of 16 QSOs in the redshift range 0.9 to 1.3. The principal points of interest are the symmetry and signs of tidal effects in the QSO hosts and nearby (`companion') galaxies. The sample…

Astrophysics of Galaxies · Physics 2009-11-13 J. B. Hutchings , P. Scholz , L. Bianchi

Low-resolution LAMOST and Keck spectra of blue supergiant stars distributed over the disks of the Local Group spiral galaxies M 31 and M 33 are analyzed to determine stellar effective temperatures, gravities, metallicities, and reddening.…

Astrophysics of Galaxies · Physics 2022-06-22 Cheng Liu , Rolf-Peter Kudritzki , Gang Zhao , Miguel A. Urbaneja , Yang Huang , Huawei Zhang , Jingkun Zhao

We discuss the sources which are likely to dominate the ionizing field throughout the Local Group. In terms of the limiting flux to produce detectable H-alpha emission (4-10 x 10**3 phot/cm**2/s), the four dominant galaxies (M31, Galaxy,…

Astrophysics · Physics 2007-05-23 J. Bland-Hawthorn

We analyse the environment of low redshift, z < 0.2, SDSS quasars using the spectral and photometric information of galaxies from the Sloan Digital Sky Survey Third Data Release (SDSS-DR3). We compare quasar neighbourhoods with field and…

Astrophysics · Physics 2009-11-11 Georgina V. Coldwell , Diego G. Lambas

We present multislit CaII near-infrared triplet spectroscopy with the Keck 10-m telescope/LRIS of 99 M31 halo red giant candidates in the apparent mag range 20<I<22 in a SE minor axis field at R=19kpc. The spectra are used to isolate M31…

Astrophysics · Physics 2009-11-07 David B. Reitzel , Puragra Guhathakurta

We compare both the Milky Way and M31 to local external disk galaxies within the same mass range, using their relative locations in the planes formed by Vflat vs. MK (the Tully-Fisher relation), j_disk (specific angular momentum) and the…

Astrophysics · Physics 2007-11-20 M. Puech , F. Hammer , L. Chemin , H. Flores , M. Lehnert