Zobrazeno 1 - 10
of 49
pro vyhledávání: '"Andrew G. Michalitsianos"'
Publikováno v:
The Astrophysical Journal. 539:111-123
Far-ultraviolet spectra of the gravitational lens components Q0957+561A, B were obtained with the Hubble Space Telescope Faint Object Spectrograph (FOS) at five equally spaced epochs, one every 2 weeks. We confirm the flux variability of the quasar's
Publikováno v:
The Astrophysical Journal. 487:L117-L120
We obtained Multiple Mirror Telescope spectra of the gravitational lens candidate UM 425 to compare the redshifts and line profile structures of lens components A and B, which are separated by approximately 65. The C IV λ1550 emission in both A and
Autor:
P. T. Boyd, Jeffrey W. Percival, Joseph F. Dolan, Frederick C. Bruhweiler, Andrew G. Michalitsianos, Robert J. Hill, M. J. Nelson, Demos Kazanas, G. W. van Citters
Publikováno v:
The Astrophysical Journal. 474:598-605
Far-ultraviolet spectra of the gravitational lens components Q0957+561A and B were obtained with the Hubble Space Telescope Faint Object Spectrograph (HST FOS). Two previously known absorption-line systems were detected at redshifts zdamped = 1.3911
Publikováno v:
Nature. 350:404-406
A dramatic change has occurred in the ultraviolet spectrum of the emission-line star MWC560, so that it now closely resembles the spectrum of a nova shortly after outburst. This event may signal a major mass-ejection episode such as presumably occurr
Autor:
P. Hintzen, Robert W. O'Connell, Theodore P. Stecher, Andrew M. Smith, Morton S. Roberts, R. C. Bohlin, Robert H. Cornett, K. P. Cheng, Andrew G. Michalitsianos, Eric P. Smith
Publikováno v:
New Aspects of Magellanic Cloud Research ISBN: 9783540564324
During the Astro-1 mission, near- and far-UV images of the 30 Doradus region were obtained using the Ultraviolet Imaging Telescope (UIT). These wide-field, 40′ in diameter, high spatial resolution, 2-3″, UIT UV images reveal a rich field of lumin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4b5e17866abdc6786de01b97a40bbe1d
https://doi.org/10.1007/3-540-56432-2_183
https://doi.org/10.1007/3-540-56432-2_183
Publikováno v:
The Astrophysical Journal. 458:67
Autor:
Joseph F. Dolan, James L. Elliot, Jeffrey W. Percival, P. T. Boyd, M. J. Nelson, G. W. van Citters, Karen G. Wolinski, M. J. Taylor, Robert Bless, R. W. Thompson, Andrew G. Michalitsianos
Publikováno v:
The Astrophysical Journal. 442:87
Photometric and polarimetric observations of both images of the gravitationally lensed quasar Q0957+561 (z(sub em) = 1.41) were obtained in the UV in 1993 with the High Speed Photometer on board the Hubble Space Photometer on board the Hubble Space T
Publikováno v:
The Astronomical Journal. 108:671
In this note, we show that the ultraviolet and optical spectroscopic variability of this unique symbiotic star can be understood in terms of a time variable collimated stellar wind with a rapid acceleration near the source. Using the radial velocitie
Publikováno v:
The Astrophysical Journal Supplement Series. 94:183
This atlas contains sample spectra from the far-ultraviolet observations of 32 symbiotic stars obtained with the International Ultraviolet Explorer (IUE) satellite. In all, 394 low-resolution spectra from the short-wavelength primary (SWP) camera cov
Autor:
Yoji Kondo, R. R. Thompson, Demos Kazanas, Stephen P. Maran, Andrew G. Michalitsianos, M. de La Pena, T. Meylan, Frederick C. Bruhweiler, M. Pérez, J. Nichols-Bohlin
Publikováno v:
The Astrophysical Journal. 417:L57
Test runs with a new data processing software system on archival spectra obtained by the International Ultraviolet Explorer (IUE) reveal high-excitation emission lines in the gravitationally lensed binary quasar 0957+561. The lines of O VI λλ1031,1