Zobrazeno 1 - 10
of 20
pro vyhledávání: '"J. E. Bowey"'
Autor:
J E Bowey, A M Hofmeister
We present new room-temperature 1100 - 1800 cm^{-1} spectra of melilite silicates and 600 - 2000 cm^{-1} spectra of three randomly orientated fine-grained carbonates to determine the possible carrier(s) of a 6.9~micron absorption feature observed in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::18b68f11f2f6cb7ab71da6b63c8a4f21
Pyroxene crystals are common in meteorites but few compositions have been recognized in astronomical environments. We present quantitative room-temperature spectra of 17 Mg-- Fe-- and Ca--bearing ortho- and clinopyroxenes, and a Ca-pyroxenoid in orde
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::67564fe7c405910d37a5938adf972956
Autor:
Mikako Matsuura, Silvia Lorenz-Martins, J. E. Bowey, Eric Lagadec, Tim Gledhill, M. J. Barlow, Hans Van Winckel, P. Bendjoya, Ryszard Szczerba, O. Suarez, T. Verhoelst, A. A. Zijlstra, Djamel Mékarnia, O. Chesneau
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 417:32-92
Post-AGB stars are key objects for the study of the dramatic morphological changes of low- to intermediate-mass stars on their evolution from the Asymptotic Giant Branch (AGB) towards the Planetary Nebula stage. There is growing evidences that binary
Autor:
Albert A. Zijlstra, Silvia Lorenz-Martins, Eric Lagadec, J. E. Bowey, Djamel Mékarnia, Olivier Chesneau, Tijl Verhoelst, Mikako Matsuura, M. J. Barlow, Philippe Bendjoya, Tim Gledhill, O. Suarez, Ryszard Szczerba, Hans Van Winckel
Publikováno v:
Proceedings of the International Astronomical Union. 7:59-62
Post-AGB stars are key objects for the study of the dramatic morphological changes of low- to intermediate-mass stars on their evolution from the Asymptotic Giant Branch (AGB) towards the planetary nebula stage. There is growing evidences that binary
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 376:1367-1374
We present mid-infrared spectra from individual enstatite silicate grains separated from primitive type 3 chondritic meteorites. The 2-16 mu m transmission spectra were taken with microspectroscopic Fourier-transform infrared (FT-IR) techniques as pa
Autor:
Per Friberg, Jeremy Yates, Gary A. Fuller, Rene Plume, Andy Gibb, John Richer, Tom J. Millar, Harold M. Butner, Marco Spaans, J. Hatchell, George F. Mitchell, J. G. A. Wouterloot, Frank Helmich, Glenn J. White, Emmanuel Caux, M. Zhu, Toby J. T. Moore, Jane V. Buckle, Serena Viti, J. E. Bowey, E. F. van Dishoeck, F. F. S. van der Tak, Cecilia Ceccarelli, Mark Thompson, Volker Ossenkopf, A. G. G. M. Tielens, M. Roellig, H. Roberts, H. E. Matthews, Michiel R. Hogerheijde, B. Weferling, Peter Schilke, J. M. C. Rawlings
Publikováno v:
Publications of the Astronomical Society of the Pacific
Publications of the Astronomical Society of the Pacific, Astronomical Society of the Pacific, 2007, 119, pp.102. ⟨10.1086/511161⟩
Publications of the Astronomical Society of the Pacific, 119(851), 102-111
Publications of the Astronomical Society of the Pacific, Astronomical Society of the Pacific, 2007, 119, pp.102. ⟨10.1086/511161⟩
Publications of the Astronomical Society of the Pacific, 119(851), 102-111
International audience; Stars form in the densest, coldest, most quiescent regions of molecular clouds. Molecules provide the only probes that can reveal the dynamics, physics, chemistry, and evolution of these regions, but our understanding of the m
Autor:
Geoffrey C. Clayton, Karl D. Gordon, Douglas L. Welch, J. E. Bowey, Margaret Meixner, Angela Speck, Tim Gledhill, Albert A. Zijlstra, Alexander G. G. M. Tielens, Nino Panagia, M. J. Barlow, Barbara Ercolano, Ben Sugerman, Martin Cohen, Martin Meyer, Michael W. Regan, J. Fabbri, Robert C. Kennicutt
Publikováno v:
Science, 313(5784), 196-200. AMER ASSOC ADVANCEMENT SCIENCE
We present late-time optical and mid-infrared observations of the Type-II supernova 2003gd in NGC 628. Mid-infrared excesses consistent with cooling dust in the ejecta are observed 499-678 days after outburst, and are accompanied by increasing optica
Autor:
Anne M. Hofmeister, J. E. Bowey
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 367:577-591
Absorption coefficients associated with atomic motions of species expected in astronomical environments are determined from infrared measurements of various hydrosilicates, hydrated magnesium oxide, and the Al-bearing chain silicate, sapphirine. Band
Autor:
Anne M. Hofmeister, J. E. Bowey
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 358:1383-1393
The distinct patterns, relatively low intensities and peak positions of overtone-combination bands of silicates and oxides suggest that the 5-8 μm spectral region can provide clues for the dust composition when near optically thick conditions exist
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 348:L13-L17
We present low resolution 10-μm spectra of the newly identified diffuse interstellar medium (ISM) sightlines towards StRS 217 and StRS 371 and a new spectrum of Cyg OB2 no. 12 obtained at the UK Infrared Telescope (UKIRT) with the Michelle imager/sp