Zobrazeno 1 - 10
of 20
pro vyhledávání: '"Cynthia J. Taylor"'
Autor:
Julie N. Skinner, Christopher S. Peters, Cynthia J. Taylor, Boris T. Gänsicke, John Southworth, John R. Thorstensen
We report follow-up spectroscopy of 29 cataclysmic variables from the Sloan Digital Sky Survey (SDSS), 22 of which were discovered by SDSS and seven other previously known systems that were recovered in SDSS. The periods for 16 of these objects were
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::572af8acb3917cf6902211f9245bac2a
Publikováno v:
Publications of the Astronomical Society of the Pacific. 116:300-310
We present spectroscopy of seven cataclysmic variable stars with orbital periods P(orb) greater than 5 hours, all but one of which are known to be dwarf novae. Using radial velocity measurements we improve on previous orbital period determinations, o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::63cc66898db04cae694030bc48885d56
https://doi.org/10.1086/382792
https://doi.org/10.1086/382792
Autor:
Holly A. Sheets, Christopher S. Peters, Julie N. Skinner, John R. Thorstensen, Cynthia J. Taylor, Kathryn E. Weil, F. A. Ringwald, Erek H. Alper
Publikováno v:
Research Notes of the AAS. 1:29
We present a table of 58 cataclysmic binary orbital periods determined using data from MDM Observatory. Most are heretofore unpublished; some are refinements of previously published periods.
Comment: One table; accepted for publication in Resear
Comment: One table; accepted for publication in Resear
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::226155e5647afdc303061c9a1d4b6de1
https://doi.org/10.3847/2515-5172/aa9d2a
https://doi.org/10.3847/2515-5172/aa9d2a
Publikováno v:
Cognition and Emotion. 15:435-452
Although cognitive theory predicts that depression-prone individuals possess negative information-processing biases, the reliable detection of this type of cognitive vulnerability has proved difficult. The present study tested the idea that depressio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6413f8ea8c4e21af63e7356a42da4c26
https://doi.org/10.1080/0269993004200169
https://doi.org/10.1080/0269993004200169
Autor:
John R. Thorstensen, Cynthia J. Taylor
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 312:629-637
We report spectroscopic orbital periods of 0.147 d (=3.53 h) for V533 Her, 0.207 d (=4.97 h) for V446 Her and 1.478 d for X Ser. V533 Her (Nova Herculis 1963) shows absorption features in its He i and Balmer lines which appear only in a limited range
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ab4c2776ff9f3f23a554d4bcbea5e440
https://doi.org/10.1046/j.1365-8711.2000.03230.x
https://doi.org/10.1046/j.1365-8711.2000.03230.x
Publikováno v:
Publications of the Astronomical Society of the Pacific. 110:1405-1411
From Ha radial velocities taken in quiescence we find orbital periods of days, 0.1591 0.0004
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8f30bc3ed9b7ed37e6f20c1bac97200e
https://doi.org/10.1086/316282
https://doi.org/10.1086/316282
Autor:
David A. Harvey, Cynthia J. Taylor, Allen W. Shafter, Seiichiro Kiyota, John R. Thorstensen, Robert E. Fried, Joseph Patterson, Jonathan Kemp, David R. Skillman, Lasse Jensen, Tonny Vanmunster
Publikováno v:
Publications of the Astronomical Society of the Pacific. 110:1290-1303
We report photometry and spectroscopy of the dwarf nova EG Cancri in its 1996/1997 episode of eruptions. The main eruption was clearly a superoutburst featuring common superhumps with a period of 0.06036(2) days, establishing the star as a new member
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e1eaccfca115a1e10b28a6b74ea1dfb5
https://doi.org/10.1086/316252
https://doi.org/10.1086/316252
Autor:
Tonny Vanmunster, David R. Skillman, Lasse Jensen, S.Y. Shugarov, Robert E. Fried, David A. Harvey, Joseph Patterson, John R. Thorstensen, Cynthia J. Taylor
Publikováno v:
Publications of the Astronomical Society of the Pacific. 110:1148-1155
We report a spectroscopic and photometric study of the novalike variable V592 Cassiopeiae (=LS I 55° 8). The spectrum is that of a typical UX UMa–type star, with weak, narrow Balmer emission superposed on broad absorption. The 0.1–2.2 μm flux d
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::cdc34cc54ddca55704f64a1022291f6e
https://doi.org/10.1086/316235
https://doi.org/10.1086/316235
Publikováno v:
The Astrophysical Journal. 491:536-544
Despite the contributions of the Hubble Space Telescope Faint Object Spectrograph (FOS) to the archive of UV observations of active galactic nuclei, the vast majority of UV reference data were obtained using the International Ultraviolet Explorer (IU
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5cefb4f5cae26c30209903c972aeefa5
https://doi.org/10.1086/305005
https://doi.org/10.1086/305005
Autor:
Eric G. Suchanek, John August Wos, Yili Wang, Biswanath De, Mitchell Anthony Delong, David Lindsey Soper, Amburgey Jack S, Glen E. Mieling, Michelle J. Dirr, Cynthia J. Taylor
Publikováno v:
ChemInform. 31
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::246ae9bd9386acbb9bf275a102d8584d
https://doi.org/10.1002/chin.200021225
https://doi.org/10.1002/chin.200021225