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Related papers: Measurements of the Singly Ionized Oxygen Auroral …

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X-ray absorption spectroscopy provides a potentially powerful tool in determining the metal abundances in various phases of the interstellar medium (ISM). We present a case study of the sight line toward 4U 1820-303 (Galactic coordinates l,…

Astrophysics · Physics 2009-11-13 Yangsen Yao , Q. Daniel Wang

We study dependence of the atmospheric $\nu_\mu$ and $\bar{\nu}_\mu$ fluxes on the deviations of the 2-3 mixing from maximal, $|45^\circ - \theta_{23}|$, on the $\theta_{23}$-octant and on the neutrino mass splitting $\Delta m_{32}^2$.…

High Energy Physics - Phenomenology · Physics 2015-03-17 Abhijit Samanta , A. Yu. Smirnov

We report multifrequency radio continuum and hydrogen radio recombination line observations of HII regions near l=24.8d b=0.1d using the Giant Metrewave Radio Telescope (GMRT) at 1.28 GHz (n=172), 0.61 GHz (n=220) and the Very Large Array…

Astrophysics · Physics 2011-08-02 N. G. Kantharia , W. M. Goss , D. Anish Roshi , Niruj R. Mohan , Francois Viallefond

Using the short-high module of the Infrared Spectrograph on the Spitzer Space Telescope, we have measured the [S IV] 10.51, [Ne II] 12.81, [Ne III] 15.56, and [S III] 18.71-micron emission lines in nine H II regions in the dwarf irregular…

We present the results of new spectral diagnostic investigations applied to high-resolution long-slit spectra of the RW Aur bipolar jet obtained with HST/STIS. The spectra include the forbidden doublets [O I] 6300,6363 \AA, [S II] 6716,6731…

Solar and Stellar Astrophysics · Physics 2015-05-14 Stanislav Melnikov , Jochen Eislöffel , Francesca Bacciotti , Jens Woitas , Thomas P. Ray

We present the results of ALMA $\sim$2 mm, $\lesssim$1$''$-resolution observations of ten (ultra)luminous infrared galaxies ([U]LIRGs; infrared luminosity $\gtrsim$ 10$^{11.7}$L$_{\odot}$) at $z <$ 0.15, targeting dense ($>$10$^{4}$…

Astrophysics of Galaxies · Physics 2022-03-02 Masatoshi Imanishi , Kouichiro Nakanishi , Takuma Izumi , Shunsuke Baba

We report on a recent spectral line survey of the planetary nebula (PN) NGC 7027 using the Arizona Radio Observatory (ARO) 12m telescope and the Heinrich Hertz Submillimeter Telescope (SMT) at millimeter wavelengths. The spectra covering…

Astrophysics · Physics 2009-11-13 Yong Zhang , Sun Kwok , Dinh-V-Trung

We aim to measure very precise and accurate model-independent masses and distances of detached binary stars. Precise masses at the $< 1$% level are necessary to test and calibrate stellar interior and evolution models, while precise and…

Solar and Stellar Astrophysics · Physics 2023-04-12 A. Gallenne , A. Mérand , P. Kervella , D. Graczyk , G. Pietrzyński , W. Gieren , B. Pilecki

Using the Tunable Diode Laser Absorption Spectroscopy (TDLAS) 82 CH$_3$I ro-vibrational overtone absorption were detected for the first time between 11660 and 11840 cm$^{-1}$ (844 -- 857 nm), with strengths estimated to be around $10^{-27}$…

Chemical Physics · Physics 2023-04-14 Alessandro Lucchesini

Extensive infrared spectra of the weakly-bound CO$_2$-CO dimer are observed in the carbon dioxide $\nu_3$ asymmetric stretch region (~2350 cm-1) using a tunable infrared OPO laser source to probe a pulsed slit jet supersonic expansion. Both…

Atomic and Molecular Clusters · Physics 2021-05-28 A. J. Barclay , A. R. W. McKellar , N. Moazzen-Ahmadi

Hyperfine structure lines of highly-charged ions may open a new window in observations of hot rarefied astrophysical plasmas. In this paper we discuss spectral lines of isotopes and ions abundant at temperatures 10^5-10^7 K, characteristic…

Astrophysics · Physics 2010-11-11 R. A. Sunyaev , D. Docenko

Optical spectra of the peculiar supergiant 3Pup taken in 1997-2008 are used to analyze the spectral peculiarities and velocity field in its atmosphere. The profiles of strong FeII lines and of the lines of other iron-group ions have a…

Solar and Stellar Astrophysics · Physics 2015-03-17 Eugenij Chentsov , Valentina Klochkova , Anatoly Miroshnichenko

Context: Recent works with improved model atmospheres, line formation, atomic and molecular data, and detailed treatment of blends, have resulted in a significant downward revision of the solar oxygen abundance. Aims: Considering the…

Astrophysics · Physics 2009-11-13 Jorge Melendez , Martin Asplund

The most accurate way to measure the energy levels for the O II 2p^3 ground configuration has been from the forbidden lines in planetary nebulae. We present an analysis of modern planetary nebula data that nicely constrain the splitting…

Astrophysics · Physics 2009-11-10 K. P. M. Blagrave , P. G. Martin

By observing the near-infrared spectrum of the quasar PG 1116+215 at z = 0.176 and combining with the HST/FOS spectrum, we obtained the relative strengths of three permitted OI lines ({lambda}1304, {lambda}8446, and {lambda}11287) in a…

Astrophysics · Physics 2015-06-24 Yoshiki Matsuoka , Shinki Oyabu , Yumihiko Tsuzuki , Kimiaki Kawara , Yuzuru Yoshii

We present the highlights from our recent study of 22 local (z$<$0.025) type-1 LINERs from the Palomar Survey, on the basis of optical long-slit spectroscopic observations taken with TWIN/CAHA, ALFOSC/NOT and HST/STIS (Cazzoli et al. 2018).…

We have discovered two simultaneous quasi-periodic oscillations (QPOs) at 898.3+/-3.3 Hz and 1158.6+/-9.0 Hz in the 1996 August 1 observation of the low-mass X-ray binary KS 1731-260 with the Rossi X-ray Timing Explorer. The rms amplitude…

Astrophysics · Physics 2009-10-30 Rudy A. D. Wijnands , Michiel van der Klis

The orbits and physical parameters of three close, double-lined G0 eclipsing binaries have been derived combining H_P, V_T, B_T photometry from the Hipparcos/Tycho mission with 8480-8740 \AA ground-based spectroscopy. The setup is mimicking…

Astrophysics · Physics 2009-11-07 T. Zwitter , U. Munari , P. M. Marrese , A. Prsa , E. F. Milone , F. Boschi , T. Tomov , A. Siviero

We present an evaluation of airborne Intensity-Modulated Continuous-Wave (IM-CW) lidar measurements of atmospheric column CO2 mole fractions during the ACT-America project. This lidar system transmits online and offline wavelengths…