Zobrazeno 1 - 10
of 28
pro vyhledávání: '"D. Y. Gezari"'
Publikováno v:
The Astrophysical Journal. 509:283-298
We have obtained array camera images of the Orion BN/KL infrared complex at nine wavelengths between 4.8 and 20 mue.
Autor:
G. G. Fazio, J. L. Hora, L. E. Allen, M. L. N. Ashby, P. Barmby, L. K. Deutsch, J.‐S. Huang, S. Kleiner, M. Marengo, S. T. Megeath, G. J. Melnick, M. A. Pahre, B. M. Patten, J. Polizotti, H. A. Smith, R. S. Taylor, Z. Wang, S. P. Willner, W. F. Hoffmann, J. L. Pipher, W. J. Forrest, C. W. McMurty, C. R. McCreight, M. E. McKelvey, R. E. McMurray, D. G. Koch, S. H. Moseley, R. G. Arendt, J. E. Mentzell, C. T. Marx, P. Losch, P. Mayman, W. Eichhorn, D. Krebs, M. Jhabvala, D. Y. Gezari, D. J. Fixsen, J. Flores, K. Shakoorzadeh, R. Jungo, C. Hakun, L. Workman, G. Karpati, R. Kichak, R. Whitley, S. Mann, E. V. Tollestrup, P. Eisenhardt, D. Stern, V. Gorjian, B. Bhattacharya, S. Carey, B. O. Nelson, W. J. Glaccum, M. Lacy, P. J. Lowrance, S. Laine, W. T. Reach, J. A. Stauffer, J. A. Surace, G. Wilson, E. L. Wright, A. Hoffman, G. Domingo, M. Cohen
The Infrared Array Camera (IRAC) is one of three focal plane instruments in the Spitzer Space Telescope. IRAC is a four-channel camera that obtains simultaneous broad-band images at 3.6, 4.5, 5.8, and 8.0 microns. Two nearly adjacent 5.2x5.2 arcmin f
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::83c00716a9be573f318f1394db9852a8
Autor:
Ronald J. Allen, Drake Deming, John D. Monnier, Sara Seager, C. Noecker, Dominic J. Benford, J. Rajagopal, S. A. Rinehart, W. A. Traub, R. Linfield, W. C. Danchi, Marc J. Kuchner, M. J. Mumma, Lee G. Mundy, D. Y. Gezari, David Leisawitz, Rafael Millan-Gabet
Publikováno v:
AIP Conference Proceedings.
The Fourier‐Kelvin Stellar Interferometer (FKSI) is a mission concept for a nulling interferometer for the near‐to‐mid‐infrared spectral region (3 – 8 μm). FKSI is conceived as a scientific and technological precursor to TPF. The scientifi
Autor:
Andreas Eckart, Koraljka Muzic, Mark Morris, D. Y. Gezari, Rainer Schoedel, Leo Meyer, Antonio Alberdi
Publikováno v:
Astronomy & Astrophysics. 532:A83
(abridged) The massive black hole at the center of the Milky Way, SagittariusA* is, in relative terms, the weakest accreting black hole accessible to observations. At the moment, the mean SED of SgrA* is only known reliably in the radio to mm regimes
Publikováno v:
The Astrophysical Journal. 409:L5
The Goddard Infrared Array Camera was used to obtain a high resolution image of the nucleus of NGC 1068 at 12.4 microns. In addition, the peak emission at 12.4 microns relative to the peak of the optical continuum was determined. The distribution of
Autor:
D. Y. Gezari, M. D. Thornley, S. R. Heap, S. N. Shore, F. Varosi, S. J. Meatheringham, S. P. Maran
Publikováno v:
Symposium - International Astronomical Union. 155:230-230
Infrared array camera images of the planetary nebula NGC7027 at seven wavelenghts between 7.8 and 20μm taken at the IRTF telescope are compared to Hα and Hβ images obtained at the CFHT, and published 2-, 6-, and 20-cm VLA maps, all made with bette
Autor:
C. M. Telesco, D. Y. Gezari
Publikováno v:
The Astrophysical Journal. 395:461
We present 12.4 micron images, made with 1" resolution, of the intense star-forming region in the galaxy M82. Considerable small-scale structure is evident, including several bright clumps less than about 20 pc in size which may be embedded with gian
A large aperture balloon-borne telescope for a submillimeter wavelength survey of the galactic plane
Autor:
L. H. Cheung, D. Walser, D. Y. Gezari, Robert F. Silverberg, A. Flanick, A. D. Silver, T. Kelsall, T. L. Skillman, J. Smith, Michael G. Hauser
Publikováno v:
Advances in Space Research. 3:139-142
A balloon-borne, 1.2 meter Cassegrain telescope with a servo-controlled chopping secondary mirror has been developed and used to survey the Galactic Plane at submillimeter wavelengths. The telescope pointing system uses a gyroscope as the primary sta
Publikováno v:
Symposium - International Astronomical Union. 87:129-132
High surface brightness 1.0 mm continuum emission has been mapped in nine southern hemisphere HII/molecular cloud complexes: NGC 6334, RCW 38, RCW 57, RCW 122, RCW 117, G333.6-0.2, G351.6-1.3, W 33 and W 33A. All of the sources are located in the inn
Autor:
G. G. Fazio, D. G. Koch, G. J. Melnick, R. M. Tresch-Fienberg, S. P. Willner, D. Y. Gezari, G. Lamb, P. Shu, G. Chin, R. Silverberg, J. Mather, W. F. Hoffmann, N. J. Woolf, J. Pipher, W. Forrest, C. R. McCreight
Publikováno v:
Instrumentation for Optical Remote Sensing from Space.