English
Related papers

Related papers: C$_{60}$ in Reflection Nebulae

200 papers

The transition strengths for the four infrared-active vibrations of charged C$_{60}$ molecules are evaluated in self-consistent density functional theory using the local density approximation. The oscillator strengths for the second and…

Condensed Matter · Physics 2009-10-28 Arthur P. Smith , George F. Bertsch

We report the measurement of infrared transmission of large C60 single crystals. The spectra exhibit a very rich structure with over 180 vibrational absorptions visible in the 100 - 4000 cm-1 range. Many silent modes are observed to have…

Condensed Matter · Physics 2009-10-22 Michael C. Martin , Xiaoqun Du , John Kwon , L. Mihaly

We present very deep CCD spectrum of the bright, medium-excitation planetary nebula NGC 7009, with a wavelength coverage from 3040 to 11000 A. Traditional emission line identification is carried out to identify all the emission features in…

Solar and Stellar Astrophysics · Physics 2015-05-27 X. Fang , X. -W. Liu

We report on the first simultaneous $NICER$ and $NuSTAR$ observations of the neutron star (NS) low-mass X-ray binary 4U 1735$-$44, obtained in 2018 August. The source was at a luminosity of $\sim1.8~(D/5.6\ \mathrm{kpc})^{2}\times10^{37}$…

We report initial results from an ongoing spectroscopic survey of central stars of faint planetary nebulae (PNe), obtained with the Low-Resolution Spectrograph on the Hobby-Eberly Telescope. The six PN nuclei (PNNi) discussed here all have…

Solar and Stellar Astrophysics · Physics 2023-03-15 Howard E. Bond , Klaus Werner , George H. Jacoby , Gregory R. Zeimann

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 present a study of McNeil's Nebula, a newly appeared reflection nebula in the L1630 cloud, together with photometry and spectroscopy of its source. New IR photometry compared to earlier 2MASS data shows that the star has brightened by…

Astrophysics · Physics 2009-11-10 Bo Reipurth , Colin Aspin

We report ALMA observations of [CI]($^3P_1-^3P_0$), C$^{13}$O, and CO$^{18}$ ($J=1-0$) toward the central region of a nearby Seyfert galaxy NGC 613. The very high resolutions of $0.26"\times0.23"(=22\times20$ pc) for [CI] and…

Astrophysics of Galaxies · Physics 2018-04-25 Yusuke Miyamoto , Masumichi Seta , Naomasa Nakai , Yoshimasa Watanabe , Dragan Salak , Shun Ishii

The infrared bar-spectrum of a single ammonia molecule encapsulated in nano-cage C$_{60}$ fullerene molecule is modelled using the site inclusion model successfully applied to analyze spectra of CO$_2$ isotopologues isolated in rare gas…

Chemical Physics · Physics 2011-03-30 Azzedine Lakhlifi , Pierre-Richard Dahoo

In this work we present VLA observations of the NH3, CCS, and H2O maser emission at 1 cm from the star forming region B1-IRS (IRAS 03301+3057) with ~ 5" (=1750 AU) of angular resolution. CCS emission is distributed in three clumps around…

ISO [C II] 158 micron, [O I] 63 micron, and H_2 9 and 17 micron observations are presented of the reflection nebula Ced 201, which is a photon-dominated region illuminated by a B9.5 star with a color temperature of 10,000 K (a cool PDR). In…

[abridged] We present multi-epoch high-resolution optical spectroscopy, UV/radio/X-ray imaging, and archival Hubble and Spitzer observations of an intermediate luminosity optical transient recently discovered in the nearby galaxy NGC300. We…

We have been able to compare with astrometric precision AstroDrizzle processed images of NGC 6720 (the Ring Nebula) made using two cameras on the Hubble Space Telescope. The time difference of the observations was 12.925 yrs. This large…

Solar and Stellar Astrophysics · Physics 2015-06-15 C. R. O'Dell , G. J. Ferland , W. J. Henney , M. Peimbert

We study the dust present in 56 Galactic planetary nebulae (PNe) through their iron depletion factors, their C/O abundance ratios (in 51 objects), and the dust features that appear in their infrared spectra (for 33 objects). Our sample…

Solar and Stellar Astrophysics · Physics 2015-06-18 Gloria Delgado-Inglada , Mónica Rodríguez

NGC 7129 is a bright reflection nebula located in the molecular cloud complex near l=105.4, b=+9.9, about 1.15 kpc distant. Embedded within the reflection nebula is a young cluster dominated by a compact grouping of four early-type stars:…

Solar and Stellar Astrophysics · Physics 2015-06-03 S. E. Dahm , L. A. Hillenbrand

Images obtained with the CTIO 4-m telescope and the MOSAIC-2 wide field camera in [O III] 5007 and H\alpha on-band and off-band filters are analyzed to search for emission lines objects in the galaxy NGC 6822. In particular we search for PN…

Astrophysics · Physics 2009-11-13 Liliana Hernandez-Martinez , Miriam Pena

We have performed a detailed spectral analysis of the inner halo Galactic globular cluster (GC) NGC 6723 using high resolution (R$\approx$ 22000-48000) spectra for for eleven red giant branch stars collected with MIKE (Magellan) and FEROS…

Solar and Stellar Astrophysics · Physics 2019-07-10 Juliana Crestani , Alan Alves-Brito , Giuseppe Bono , Arthur A. Puls , Javier Alonso-García

We have combined recent Hubble Space Telescope WFPC2 images in the [O III] 5007 and [N II] 6583 lines with similar images made 9.557 years earlier to determine the motion of the Ring Nebula within the plane of the sky. Scaled ratio images…

Astrophysics of Galaxies · Physics 2009-11-13 C. R. O'Dell , W. J. Henney , F. Sabbadin

We present Spitzer high-resolution spectra of off-nuclear regions in the central cluster galaxies NGC 1275 and NGC 4696 in the Perseus and Centaurus clusters, respectively. Both objects are surrounded by extensive optical emission-line…

Astrophysics · Physics 2009-11-13 R. Johnstone , N. Hatch , G. Ferland , A. Fabian , C. Crawford , R. Wilman

We report here results on the long time behaviour of the variable source 4U 1722-30, obtained from INTEGRAL non-continuous observations carried out between 2003 and 2009. During this period 4U 1722-30 shows a general persistent emission…

High Energy Astrophysical Phenomena · Physics 2013-03-15 Antonella Tarana , Angela Bazzano , Pietro Ubertini