Zobrazeno 1 - 10
of 129
pro vyhledávání: '"E. M. Burbidge"'
Publikováno v:
Publications of the Astronomical Society of the Pacific. 118:124-128
The galaxy cluster RX J0152.7−1357 at \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,x
Publikováno v:
The Astrophysical Journal. 620:88-94
A strong X-ray source only 8" from the nucleus of the Sy2 galaxy NGC 7319 in Stephan's Quintet has been discovered by Chandra. We have identified the optical counterpart and show it is a QSO with $z_e = 2.114$. It is also a ULX with $L_x = 1.5 x 10^{
Autor:
E. M. Burbidge, R. W. Lyons, Grzegorz Madejski, E. A. Beaver, Vesa T. Junkkarinen, Ross D. Cohen
Publikováno v:
The Astrophysical Journal. 614:658-670
We present new HST STIS NUV-MAMA and STIS CCD observations of the BL Lac object AO 0235+164 and the intervening damped Ly alpha (DLA) line at z_a = 0.524. The line profile gives N(H I) = 5 +/- 1 x 10^{21} cm^{-2} and, combined with the H I 21 cm abso
Publikováno v:
The Astrophysical Journal. 591:690-694
The starburst / AGN galaxy M82 was studied by Dahlem, Weaver and Heckman using X-ray data from ROSAT and ASCA, as part of their X-ray survey of edge-on starburst galaxies. They found seventeen unresolved hard-X-ray sources around M82, in addition to
Publikováno v:
Astronomy & Astrophysics. 391:833-840
NGC3628 is a well-studied starburst/low level AGN galaxy in the Leo Triplet noted for its extensive outgassed plumes of neutral hydrogen. QSOs are shown to be concentrated around NGC3628 and aligned with the HI plumes. The closest high redshift quasa
Autor:
E. M. Burbidge, Geoffrey Burbidge
Publikováno v:
Publications of the Astronomical Society of the Pacific. 114:253-256
New spectrophotometric observations are presented for three blue stellar objects pinpointed as candidate optical identifications of ROSAT X‐ray point sources in the field around the Seyfert 1 galaxy NGC 5548. They are shown to be medium‐redshift
Autor:
E. M. Burbidge, Ross D. Cohen, D. M. Crenshaw, Vesa T. Junkkarinen, Fred Hamann, Joseph C. Shields
Publikováno v:
The Astrophysical Journal. 496:761-774
NeVIII 774 is an important tracer of the high-ionization gas in QSOs. We examine the NeVIII emission-line properties using new HST-FOS spectra of four sources, mean spectra derived from two QSO samples in the HST archives, and new photoionization cal
Publikováno v:
The Astrophysical Journal. 478:80-86
We discuss high-resolution (~9 km s-1) Keck Observatory spectra of the associated (za ≈ ze) absorption lines in the ze = 2.15 QSO UM 675. In a previous paper we showed that the time-variable absorption lines require a minimum gas density of ~4000 c
Publikováno v:
International Astronomical Union Colloquium. 159:96-103
We describe two ongoing studies of QSO broad emissionline regions (BELRs). The first employs the N V λ1240/He II λ1640 and N V/C IV λ1549 line ratios as diagnostics of QSO metallicities. Hamann & Ferland and Ferland et al. showed that many observe
Publikováno v:
The Astrophysical Journal. 553:L11-L13
Four compact ROSAT X-ray sources very close to the nearby ultraluminous infrared galaxy Arp 220 (IC 4553) have been identified as medium-redshift QSOs. The closest pair lying symmetrically across the galaxy have almost identical redshifts z = 1.25, 1