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In order to understand the evolutionary status of the anomalous supergiant UUHer, the prototype of the class of variable supergiants located at high galactic latitudes, we obtained several high-resolution spectra of this star, with the 6m…

Astrophysics · Physics 2007-05-23 V. G. Klochkova , V. E. Panchuk , E. L. Chentsov

The absorption of stellar radiation observed by the HD209458b in resonant lines of OI and CII has not yet been satisfactorily modeled. In our previous 2D simulations we have shown that the hydrogen-dominated upper atmosphere of HD209458b,…

Earth and Planetary Astrophysics · Physics 2020-06-14 I F Shaikhislamov , M L Khodachenko , H Lammer , A G Berezutsky , I B Miroshnichenko , M S Rumenskikh

High spectral resolution mid-IR observations of ethylene (C2H4) towards the AGB star IRC+10216 were obtained using the Texas Echelon Cross Echelle Spectrograph (TEXES) at the NASA Infrared Telescope Facility (IRTF). Eighty ro-vibrational…

Solar and Stellar Astrophysics · Physics 2017-02-08 J. P. Fonfria , K. H. Hinkle , J. Cernicharo , M. J. Richter , M. Agundez , L. Wallace

Wisconsin H-Alpha Mapper (WHAM) observations reveal high-velocity and [NII]$\lambda6584$ emission lines in the same direction and velocity as ultraviolet absorption-line features that have been previously associated with the biconical…

Astrophysics of Galaxies · Physics 2020-08-19 Dhanesh Krishnarao , Robert A. Benjamin , L. Matthew Haffner

Model atmosphere fits to high-resolution optical spectra of Wray 977 confirm the B hypergiant classification of the massive companion to the X-ray pulsar GX301-2. The models give a radius of 62 Rsun, an effective temperature of 18,100 K and…

Astrophysics · Physics 2009-11-11 L. Kaper , A. van der Meer , F. Najarro

We have recently discovered a supermassive binary black hole system with a projected separation between the two black holes of 7.3 parsecs in the radio galaxy 0402+379. This is the most compact supermassive binary black hole pair yet imaged…

Cosmology and Nongalactic Astrophysics · Physics 2010-01-15 C. Rodriguez , G. B. Taylor , R. T. Zavala , Y. M. Pihlstrom , A. B. Peck

We report R~3000 VLT ISAAC K-band spectroscopy of the nuclei (i.e. central 100-300pc) of 9 galaxies hosting an active galactic nucleus. For 5 of these we also present spectra of the circumnuclear region out to 1kpc. We have measured a…

Astrophysics · Physics 2009-11-13 R. I. Davies , A. Sternberg , M. D. Lehnert , L. E. Tacconi-Garman

We analyse absorption characteristics and physical conditions of extraplanar intermediate- and high-velocity gas to study the distribution of the neutral and weakly ionised Milky Way halo gas and its relevance for the evolution of the Milky…

Astrophysics · Physics 2015-05-13 N. Ben Bekhti , P. Richter , T. Westmeier , M. T. Murphy

We have detected HI 21cm line absorption by the Warm Neutral Medium (WNM) using the Westerbork Synthesis Radio Telescope. The absorption was detected toward Cygnus A at LSR velocities of -40 and -70 km s^{-1}. These two velocity ranges were…

Astrophysics · Physics 2009-10-30 C. L. Carilli , K. S. Dwarakanath , W. M. Goss

We present Far Ultraviolet Spectroscopic Explorer and Space Telescope Imaging Spectrograph observations of high-ionization interstellar absorption toward HD 14434 [(l, b) = (135.1, -3.8); d ~ 2.3 kpc], an O5.5 V star in the Perseus OB1…

Optical observations from 1989 of the SMC B[e] supergiant star S23 revealed the presence of photospheric HeI absorption lines. In our high-resolution optical spectra from 2000, however, we could not identify any HeI line. The observed…

We present the analysis of 200 high-resolution and 150 low-resolution spectra of the pulsating subdwarf close binary KPD 1930+2752 obtained with the Keck and the Calar Alto 2.2 m telescopes. Using metal-rich, line blanketed LTE model…

Astrophysics · Physics 2007-05-23 S. Geier , U. Heber , N. Przybilla , R. P. Kudritzki

We present 21-cm HI line and 13-cm continuum observations, obtained with the Australian Long Baseline Array, of the Seyfert 2 galaxy IC 5063. This object appears to be one of the best examples of Seyfert galaxies where shocks produced by…

Astrophysics · Physics 2009-10-31 T. A. Oosterloo , R. Morganti , A. Tzioumis , J. Reynolds , E. King , P. McCulloch , Z. Tsvetanov

Using the upGREAT instrument on SOFIA, we have imaged [C II] 157.74 and [O I] 63.18 micron line emission from a bright photodissociation region (PDR) associated with an ionized ``bubble'' located in the Nessie Nebula, a filamentary infrared…

We analyze optical and near infrared spectra of intermediate and high resolution of the eclipsing symbiotic system AR Pavonis. We have obtained the radial velocity curves for the red and the hot component from the M-giant absorption lines…

Astrophysics · Physics 2009-11-07 C. Quiroga , J. Mikolajewska , E. Brandi , O. Ferrer , L. Garcia

We present the results of adaptive optics nulling interferometric observations of two Herbig Ae stars, AB Aur and V892 Tau. Our observations at 10.3 microns show resolved circumstellar emission from both sources. Further analysis of the AB…

Astrophysics · Physics 2009-11-10 W. M. Liu , P. M. Hinz , W. F. Hoffmann , G. Brusa , D. Miller , M. A. Kenworthy

We report on our observations of the 79 and 119um doublet transitions of OH for 24 local (z<0.262) ULIRGs observed with Herschel-PACS as part of the Herschel ULIRG Survey (HERUS). Some OH119 profiles display a clear P-Cygni shape and…

The discovery of a previously unknown 21cm HI line source identified as an ultra-compact high velocity cloud in the ALFALFA survey is reported. The HI detection is barely resolved by the Arecibo 305m telescope ~4' beam and has a narrow HI…

B[e] supergiants and yellow hypergiants share a number of common properties regarding their circumstellar environments. Using the forbidden [O I] and [Ca II] lines as disk tracers, we suggest the presence of a Keplerian disk or ring around…

Solar and Stellar Astrophysics · Physics 2016-11-21 Anna Aret , Michaela Kraus , Indrek Kolka , Grigoris Maravelias

We present new Karl G. Jansky Very Large Array radio continuum images of the nuclei of Arp 220, the nearest ultra-luminous infrared galaxy. These images have both the angular resolution to study detailed morphologies of the two nuclei that…