中文
相关论文

相关论文: OI and CaII observations in intermediate redshift …

200 篇论文

We used Spitzer/IRS spectroscopic data on 426 galaxies including quasars, Seyferts, LINER and HII galaxies to investigate the relationship among the mid-IR emission lines. There is a tight linear correlation between the [Ne V]14.3 um and…

宇宙学与河外天体物理 · 物理学 2015-05-20 Miguel Pereira-Santaella , Aleksandar M. Diamond-Stanic , Almudena Alonso-Herrero , George H. Rieke

In order to test the unified scheme for luminous radio galaxies and quasars we observed 10 galaxy/quasar pairs from the 3CR catalogue with ISOPHOT at infrared wavelengths between 5 and 180 micron. Each pair was selected such that both the…

天体物理学 · 物理学 2009-11-06 K. Meisenheimer , M. Haas , S. A. H. Müller , R. Chini , U. Klaas , D. Lemke

We present an analysis of interstellar Na I (lambda=3302.37\AA, 3302.98\AA), Ti II (lambda=3383.76\AA) and Ca II K (lambda=3933.66\AA) absorption features for 74 sightlines towards O- and B-type stars in the Galactic disc. The data were…

天体物理学 · 物理学 2009-11-11 I. Hunter , J. V. Smoker , F. P. Keenan , C. Ledoux , E. Jehin , R. Cabanac , C. Melo , S. Bagnulo

The CIII] and CIV rest-frame UV emission lines are powerful probes of the ionizations states of galaxies. They have furthermore been suggested as alternatives for spectroscopic redshift confirmation of objects at the epoch of reionization…

Absorption along quasar sightlines remains among the most sensitive direct measures of HeII reionization in much of the intergalactic medium (IGM). Until recently, fewer than a half-dozen unobscured quasar sightlines suitable for the HeII…

宇宙学与河外天体物理 · 物理学 2014-11-20 David Syphers , Scott F. Anderson , Wei Zheng , Daryl Haggard , Avery Meiksin , Donald P. Schneider , Donald G. York

We use the coadded spectra of 32 epochs of Sloan Digital Sky Survey (SDSS) Reverberation Mapping Project observations of 482 quasars with z>1.46 to highlight systematic biases in the SDSS- and BOSS-pipeline redshifts due to the natural…

星系天体物理 · 物理学 2016-12-14 K. D. Denney , Keith Horne , W. N. Brandt , C. J. Grier , Luis C. Ho , B. M. Peterson , J. R. Trump , J. Ge

We analyze VLT/X-shooter data for 7 quasars, where we study the relationships between their broad absorption line (BAL) and emission line outflows. We find: 1) the luminosity of the [OIII] $\lambda$5007 emission profile decreases with…

星系天体物理 · 物理学 2020-05-13 Xinfeng Xu , Nadia Zakamska , Nahum Arav , Timothy Miller , Chris Benn

The HeII transverse proximity effect -- enhanced HeII Ly$\alpha$~transmission in a background sightline caused by the ionizing radiation of a foreground quasar -- offers a unique opportunity to probe the morphology of quasar-driven HeII…

星系天体物理 · 物理学 2017-10-04 Tobias M. Schmidt , Gabor Worseck , Joseph F. Hennawi , J. Xavier Prochaska , Neil H. M. Crighton

Understanding the links between different phases of outflows from active galactic nuclei is a key goal in extragalactic astrophysics. Here we compare [OIII] $\lambda\lambda$4960,5008 outflow signatures in quasars with and without Broad…

We present a multiwavelength spectral study of the quasar HE0359-3959, which has been identified as an extreme radiating source at intermediate redshift (z=1.5209). Along the spectral range, the different ionic species give information…

We present three-dimensional astrochemical simulations and synthetic observations of magnetised, turbulent, self-gravitating molecular clouds. We explore various galactic interstellar medium environments, including cosmic-ray ionization…

星系天体物理 · 物理学 2021-01-20 Thomas G. Bisbas , Jonathan C. Tan , Kei E. I. Tanaka

Measurements are presented and analyzed of the strength of the Ca II triplet lines in red giants in Galactic globular and open clusters, and in a sample of red giants in the LMC disk that have significantly different [Ca/Fe] abundance…

太阳与恒星天体物理 · 物理学 2015-11-11 G. S. Da Costa

We present analysis of observations of CO2 and OI emission in three comets to measure the CO2 abundance and evaluate the possibility of employing observations of OI emission in comets as a proxy for CO2. We obtained NIR imaging sensitive to…

We have obtained deep optical, long-slit spectrophotometry of the Galactic HII regions M 17, NGC 3576 and of the Magellanic Cloud HII regions 30 Doradus, LMC N11B and SMC N66, recording the optical recombination lines (ORLs) of CII, NII and…

天体物理学 · 物理学 2009-11-07 Yiannis G. Tsamis , M. J. Barlow , X. -W. Liu , I. J. Danziger , P. J. Storey

We report results of a search for CIII] $\lambda \lambda$1907,1909 {\AA} emission using Keck's MOSFIRE spectrograph in a sample of 7 $z_{phot}\sim7-8$ candidates ($H\sim27$) lensed by the Hubble Frontier Field cluster Abell 2744. Earlier…

星系天体物理 · 物理学 2015-05-27 Adi Zitrin , Richard S. Ellis , Sirio Belli , Dan P. Stark

We present a new, high resolution HST/GHRS spectrum of quasar Q0302-003, and use the HeII Lyman-$\alpha$ absorption, together with a high resolution Keck spectrum of the HI Lyman-$\alpha$ forest, to probe the distribution and ionization…

天体物理学 · 物理学 2009-09-28 Craig J. Hogan , Scott F. Anderson , Martin H. Rugers

We have used spectra of 181 projected quasar pairs at separations $\le 1.5$ arcmins from the Sloan Digital Sky-Survey Data Release 12 in the redshift range of 2.5 to 3.5 to probe the proximity regions of the foreground quasars. We study the…

星系天体物理 · 物理学 2019-11-06 Priyanka Jalan , Hum Chand , Raghunathan Srianand

We present the analysis of optical and near-infrared spectra of the only four $z>6.5$ quasars known to date, discovered in the UKIDSS-LAS and VISTA-VIKING surveys. Our data-set consists of new VLT/X-Shooter and Magellan/FIRE observations.…

The Ly-alpha absorption spectrum of the highest redshift quasars indicates that they are surrounded by giant HII regions, a few Mpc in size. The neutral gas around these HII regions should emit 21cm radiation in excess of the Cosmic…

天体物理学 · 物理学 2009-11-10 Stuart Wyithe , Abraham Loeb

We present Keck/MOSFIRE $H$-band spectroscopy targeting C$\,$III] $\lambda$1907,1909 in a $z=7.5056$ galaxy previously identified via Ly$\alpha$ emission. We detect strong line emission at $1.621\pm0.002\,\mu$m with a line flux of…