Zobrazeno 1 - 10
of 39
pro vyhledávání: '"Donald Hoard"'
Autor:
Steve B. Howell, Robert O. Harmon, Donald Hoard, Justin Ely, John H. Debes, Rachael M. Roettenbacher
Publikováno v:
The Astronomical Journal. 156:119
We analyze extensive ground- and space-based ultraviolet-infrared observations of the variable white dwarf BOKS 53856. Photometry and spectroscopy were obtained from the Hubble Space Telescope, Spi ...
Publikováno v:
Astrophysical Journal
Artículos CONICYT
CONICYT Chile
instacron:CONICYT
Artículos CONICYT
CONICYT Chile
instacron:CONICYT
We present ISAAC spectroscopy and ISAAC, UKIDSS and Spitzer Space Telescope broad-band photometry of SDSS J1228+1040 -- a white dwarf for which evidence of a gaseous metal-rich circumstellar disk has previously been found from optical emission lines.
Publikováno v:
The Astronomical Journal. 132:1989-1994
We present four MIPS (24 \micron) and two IRAC (3.6, 4.5, 5.8, and 8.0 \micron) Spitzer observations of the newly discovered Tremendous Outburst Amplitude Dwarf nova (TOAD) Var Her 04 during decline from super-outburst. The four MIPS observations spa
Autor:
Bing Chen, Gary D. Schmidt, Scott F. Anderson, Paula Szkody, J. Brinkmann, Arne Henden, Donald Hoard, Wolfgang Voges, Lee Homer
Publikováno v:
The Astronomical Journal. 128:2443-2447
XMM-Newton observations of the polar SDSSJ155331.12+551614.5 reveal that all the X-ray flux emerges at energies less than 2 keV. The best fit to the spectrum is with a thermal plasma with kT=0.8 keV plus a 20-90 ev black body, yielding a thermal X-ra
Autor:
Donald Hoard, Paula Szkody, K. Nishikida, Edward M. Sion, Knox S. Long, Anil C. Seth, John C. Raymond
Publikováno v:
The Astrophysical Journal. 574:942-949
We have observed the prototypical dwarf nova U Gem at quiescence with the Chandra medium- and high-resolution gratings to accomplish the first study of resolved X-ray emission lines in a disk-accreting cataclysmic variable. Doppler tomograms construc
Autor:
Rodolfo Montez, Andrew C. Layden, Gabriel Brammer, Donald Hoard, Shadrian Holmes, Jorge Cuadra, Kathy L. Cooksey, Alicia S. Day, Erika Labbe
Publikováno v:
Publications of the Astronomical Society of the Pacific. 114:645-649
We present light curves in the B, V, and I passbands for six field RR Lyrae stars. We derive the stars' intensity‐mean magnitudes, light amplitudes, and colors at minimum light. We compare the latter with measurements from other variables and discu
Publikováno v:
Publications of the Astronomical Society of the Pacific. 112:1595-1606
We present an analysis of ground-based optical photometry and spectroscopy, and Rossi X-ray Timing Explorer X-ray observations of the old novae DI Lacertae and V841 Ophiuchi. Our optical photometry data (obtained with the automated photometry telesco
Autor:
Paula Szkody, Vandana Desai, Donald Hoard, Boris T. Gänsicke, Robert E. Fried, Todd Burdullis, Peter M. Garnavich
Publikováno v:
The Astrophysical Journal. 540:983-991
To explore the amount of secondary irradiation and the long-term effects of a superoutburst (SOB) on tremendous outburst amplitude dwarf novae (TOADs), we obtained spectra of EG Cnc for 3-17 months past its SOB, of SW UMa, WX Cet, and USNO 1425.09823
Publikováno v:
The Astrophysical Journal. 539:L49-L53
We present the ultraviolet spectrum of the SW Sextantis star and nova-like variable DW Ursae Majoris in an optical low state, as observed with the Space Telescope Imaging Spectrograph on board the Hubble Space Telescope (HST). The data are well descr
Publikováno v:
The Astronomical Journal. 119:365-368
Three nights of blue and red spectroscopy of the extreme-amplitude dwarf nova GW Lib at quiescence show that the orbital period is 79.4 minutes and the semiamplitude of the Hβ emission-line velocity curve is 40.0 km s-1. The emission lines are very