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相关论文: Drastic changes in the molecular absorption at red…

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New millimeter wave observations of the molecular absorption line system in the gravitational lens to PKS1830-211 at z=0.88582 is presented. Self-calibrated interferometer data shows unequivocally that the previously detected absorption…

天体物理学 · 物理学 2009-10-30 Tommy Wiklind , Francoise Combes

Based on measurements with the Effelsberg 100-m telescope, a multi-line study of molecular species is presented toward the south-western source of the gravitational lens system PKS 1830-211, which is by far the best known target to study…

星系天体物理 · 物理学 2015-02-04 A. Schulz , C. Henkel , K. M. Menten , S. Muller , D. Muders , J. Bagdonaite , W. Ubachs

Time variability of astronomical sources provides crude information on their typical size and on the implied physical mechanisms. PKS1830-211 is a remarkable radio-bright lensed quasar with a foreground molecular absorber at z=0.89.…

星系天体物理 · 物理学 2024-09-02 S. Muller , I. Marti-Vidal , F. Combes , M. Gerin , A. Beelen , C. Horellou , M. Guelin , S. Aalto , J. H. Black , E. van Kampen

With the Plateau de Bure interferometer, we have measured the C, N, O and S isotopic abundance ratios in the arm of a spiral galaxy with a redshift of 0.89. The galaxy is seen face-on according to HST images. Its bulge intercepts the line…

天体物理学 · 物理学 2009-11-11 Sebastien Muller , Michel Guelin , Michael Dumke , Robert Lucas , Francoise Combes

Optical and near-IR Hubble Space Telescope and Gemini-North adaptive optics images, further improved through deconvolution, are used to explore the gravitationally lensed radio source PKS 1830-211. The line of sight to the quasar at z=2.507…

天体物理学 · 物理学 2009-11-07 F. Courbin , G. Meylan , J. P. Kneib , C. Lidman

This paper presents data from the BIMA interferometer showing spatially resolved absorption spectra of the gravitationally lensed quasar PKS 1830-211. High-resolution (1.2 km/s) spectra were taken in two spectral windows centered on the…

天体物理学 · 物理学 2009-11-06 J. Swift , W. J. Welch , B. Frye

We present the results of a 7 mm spectral survey of molecular absorption lines originating in the disk of a z=0.89 spiral galaxy located in front of the quasar PKS 1830-211. [...] A total of 28 different species, plus 8 isotopic variants,…

宇宙学与河外天体物理 · 物理学 2015-05-27 S. Muller , A. Beelen , M. Guélin , S. Aalto , J. H. Black , F. Combes , S. Curran , P. Theule , S. Longmore

We present the first results of an ALMA spectral survey of strong absorption lines for common interstellar species in the z=0.89 molecular absorber toward the lensed blazar PKS1830-211. The dataset brings essential information on the…

We report the first science observations and results obtained with the "extended" SMA (eSMA), which is composed of the SMA (Submillimeter Array), JCMT (James Clerk Maxwell Telescope) and CSO (Caltech Submillimeter Observatory). Redshifted…

We report the detection of molecular absorption lines at z=0.7645 towards the radio-loud QSO PMN 0134-0931. The CO J=2-1 and HCO+ J=2-1 lines are seen in absorption along two different lines of sight to lensed images of the background QSO.…

星系天体物理 · 物理学 2018-09-05 Tommy Wiklind , Françoise Combes , Nissim Kanekar

We present the first detections of CH3SH, C3H+, C3N, HCOOH, CH2CHCN, and H2CN in an extragalactic source. Namely the spiral arm of a galaxy located at z=0.89 on the line of sight to the radio-loud quasar PKS 1830-211. OCS, SO2, and NH2CN…

星系天体物理 · 物理学 2020-04-29 B. Tercero , J. Cernicharo , S. Cuadrado , P. de Vicente , M. Guélin

The line of sight to the quasar B0218+357, one of the most studied lensed systems, intercepts a z=0.68 spiral galaxy, which splits its image into two main components A and B, separated by ca. 0.3'', and gives rise to molecular absorption.…

天体物理学 · 物理学 2009-11-13 S. Muller , M. Guelin , F. Combes , T. Wiklind

We have detected the J=4-3 rotational transition of 12CO in absorption at z=0.89 towards the quasar PKS1830-211, but not the 12CO 5-4 or the 3P1-3P0 fine structure line of neutral carbon. The intervening molecular medium thus has a total…

天体物理学 · 物理学 2009-10-30 M. Gerin , T. G. Phillips , D. J. Benford , K. H. Young , K. M. Menten , B. Frye

We present X-ray spectral analysis of five Chandra and XMM-Newton observations of the gravitationally-lensed blazar PKS1830-211 from 2000 to 2004. We show that the X-ray absorption toward PKS1830-211 is variable, and the variable absorption…

天体物理学 · 物理学 2009-06-23 Xinyu Dai , Smita Mathur , George Chartas , Sunita Nair , Gordon P. Garmire

PKS1830-211 is an unusually radio-loud gravitationally lensed quasar. In the radio, the system appears as two compact, dominant features surrounded by relatively extended radio emission which forms an Einstein Ring. As the line of sight to…

天体物理学 · 物理学 2016-08-30 Smita Mathur , Sunita Nair

We have made radio- and millimeter-wavelength interferometric observations of a variety of molecular absorption lines toward the gravitational lens systems B0218+357 and PKS1830-211. The absorption occurs in the lensing galaxies at…

天体物理学 · 物理学 2007-05-23 Karl M. Menten , Christopher L. Carilli , Mark J. Reid

We report the detection of 21-cm absorption from foreground galaxies towards quasars, specifically z_gal = 0.3120 towards SDSS J084957.97+510829.0 (z_qso = 0.584; Pair-I) and z_gal = 0.3714 towards SDSS J144304.53+021419.3 (z_qso = 1.82;…

星系天体物理 · 物理学 2015-06-16 N. Gupta , R. Srianand , P. Noterdaeme , P. Petitjean , S. Muzahid

A detailed study of the absorbing molecular clouds towards the radio source PKS1413+135, at a redshift z=0.247, is reported. Physical conditions are derived for the molecular gas in the frame work of two models: a homogeneous multicomponent…

天体物理学 · 物理学 2007-05-23 Tommy Wiklind , Francoise Combes

CRTS J084133.15+200525.8 is an optically bright quasar at z=2.345 that has shown extreme spectral variability over the past decade. Photometrically, the source had a visual magnitude of V~17.3 between 2002 and 2008. Then, over the following…

Westerbork Radio Synthesis Telescope observations of the redshifted 21cm line absorber against the z_em = 0.871 double lobed quasar 3C196 show that the intervening absorber is an L approximately equal L* spiral galaxy (3C196-G1) and that…

天体物理学 · 物理学 2009-11-06 F. H. Briggs , A. G. de Bruyn , R. C. Vermeulen
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