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Related papers: Extended CIII]lambda1909 emission in Q0957+561

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We present an analysis of HI Lyman-alpha emission in deep VLT/MUSE observations of two highly magnified and extended galaxies at z=3.5 and 4.03, including a newly discovered, almost complete Einstein ring. While these Lyman-alpha haloes are…

We announce the discovery of an extended emission line region associated with a high redshift type-2 QSO. The halo, which was discovered in our new wide-field narrow-band survey, resides at z = 2.85 in the Spitzer First Look Survey region…

Astrophysics · Physics 2009-11-13 Daniel J. B. Smith , Matt J. Jarvis , Chris Simpson , Alejo Martinez-Sansigre

We analysed new wide-field, wide- and narrow-band optical images of IC 59 and IC 63, two nebulae which are externally illuminated by the early B-star {\gamma} Cas, with the objective of mapping the extended red emission (ERE), a…

Astrophysics of Galaxies · Physics 2017-05-12 Thomas S. -Y. Lai , Adolf N. Witt , Ken Crawford

Using ALMA, we report high angular-resolution observations of the redshift z=3.63 galaxy, G09v1.97, one of the most luminous strongly lensed galaxies discovered by the H-ATLAS survey. We present 0"2-0"4 resolution images of the rest-frame…

We present results of HST observations of the radio galaxy 3C 299. The broad-band F702W (R) and F555W (V) images (WFPC2/PC) show an elliptical galaxy, with a comet-like structure extending to the NE in the radio jet direction. The…

Line profile distortions are commonly observed in gravitationally lensed quasar spectra. These distortions are caused by microlensing from the stars in the lensing galaxy, which produce differential magnification of spatially and…

Astrophysics of Galaxies · Physics 2021-10-27 Damien Hutsemékers , Dominique Sluse

We present the results of BVRI imaging and optical spectroscopy of the dwarf galaxy A0951+68. The images reveal that, although this galaxy is classified as a dwarf elliptical, it has some properties that are similar to dwarf irregular…

Astrophysics · Physics 2015-06-24 R. A. Johnson , A. Lawrence , R. Terlevich , D. Carter

We determine abundances from the absorption spectrum of the magnetic Herbig Ae star HD 190073 (V1295 Aql). The observations are primarily from HARPS spectra obtained at a single epoch. We accept arguments that the presence of numerous…

Solar and Stellar Astrophysics · Physics 2015-06-03 C. R. Cowley , S. Hubrig

We report an increase of more than 0.2 mag in the optical brightness of the leading image (A) of the gravitational lens Q0957+561, detected during the 09/2000 -- 06/2001 monitoring campaign (2001 observing season). The brightening is…

Astrophysics · Physics 2009-11-07 A. Oscoz , D. Alcalde , M. Serra-Ricart , E. Mediavilla , J. A. Munoz

We locate the gamma-ray and lower frequency emission in flares of the BL Lac object AO 0235+164 at >12pc in the jet of the source from the central engine. We employ time-dependent multi-spectral-range flux and linear polarization monitoring…

We have discovered extended X-ray emission from the microquasar Cyg X-3 in archival Chandra X-ray Observatory observations. A 5" wide structure lies approximately 16" to the NE from the core point source and may be extended in that…

Astrophysics · Physics 2009-11-07 W. A. Heindl , J. A. Tomsick , R. Wijnands , D. M. Smith

We report preliminary results from a targeted investigation on quasars containing damped Lyman-alpha absorption (DLA) lines as well strong metal absorption lines, carried out with the Potsdam Multi Aperture Spectrophotometer (PMAS). We…

Astrophysics · Physics 2009-11-10 L. Christensen , S. F. Sanchez , K. Jahnke , T. Becker , A. Kelz , L. Wisotzki , M. M. Roth

Based on additional interferometric observations, we reanalysed the CO(2-1) and 3mm continuum emission of Q0957+561, a lensed QSO at a redshift of z=1.4141. The emission in the CO(2-1) lines reveals a gas-rich host galaxy with a peculiar…

Astrophysics · Physics 2016-08-30 M. Krips , R. Neri , A. Eckart , D. Downes , J. Martin-Pintado , P. Planesas

We present spatially resolved Alma Band-9 observations of the [CII] 158 $\mu$m fine structure line from an optically selected quasar, SDSS J100038.01+020822.4 (J1000), at z=1.8275. By utilizing [OI] 63 $\mu$m line observations from…

We have discovered an extended Lyman alpha plume associated with a compact source at redshift 5.4 in slitless spectroscopic data from the Grism ACS Program for Extragalactic Science (GRAPES) project. The spatial extent of the emission is…

Emission-line stars are typically surrounded by dense circumstellar material, often in form of rings or disc-like structures. Line emission from forbidden transitions trace a diversity of density and temperature regimes. Of particular…

Solar and Stellar Astrophysics · Physics 2016-01-27 Anna Aret , Michaela Kraus , Miroslav Šlechta

We present echelle spectrophotometry of the Galactic H II region S 311. The data have been taken with the Very Large Telescope UVES echelle spectrograph in the 3100 to 10400 angstroms range. We have measured the intensities of 263 emission…

Astrophysics · Physics 2009-11-13 J. Garcia-Rojas , C. Esteban , A. Peimbert , M. Peimbert , M. Rodriguez , M. T. Ruiz

(abridged abstract) We present multi-epoch high-resolution spectroscopy and photoelectric polarimetry of the long-period polar (AM Herculis star) QQ Vul. The blue emission lines show several distinct components, the sharpest of which can…

J1004+4112 is a lensed quasar for which the first broad emission line profile deformations due to microlensing were identified. Detailed interpretations of these features have nevertheless remained controversial. Based on 15 spectra…

Astrophysics of Galaxies · Physics 2023-03-29 Damien Hutsemékers , Dominique Sluse , Đorđe Savić , Gordon T. Richards

High resolution observations in the region of the lines Halpha, He II 4686 and Hgamma of the spectrum of the symbiotic binary Z And were performed during its small-amplitude brightening at the end of 2002. The profiles of the hydrogen lines…

Solar and Stellar Astrophysics · Physics 2015-05-18 N. A. Tomov , M. T. Tomova , D. V. Bisikalo
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