AAAAAA

   
Results: 1-8 |
Results: 8
Interferometric astrometry with Hubble Space Telescope fine guidance sensor 3: The parallax of the cataclysmic variable TV Columbae
Authors: McArthur, BE Benedict, GF Lee, J van Altena, WF Slesnick, CL Rhee, J Patterson, RJ Frederick, LW Harrison, TE Spiesman, WJ Nelan, E Duncombe, RL Hemenway, PD Jefferys, WH Shelus, PJ Franz, OG Wasserman, LH
Citation: Be. Mcarthur et al., Interferometric astrometry with Hubble Space Telescope fine guidance sensor 3: The parallax of the cataclysmic variable TV Columbae, ASTROPHYS J, 560(2), 2001, pp. 907-911
Precise masses for Wolf 1062 AB from Hubble Space Telescope interferometric astrometry and McDonald Observatory radial velocities
Authors: Benedict, GF McArthur, BE Franz, OG Wasserman, LH Henry, TJ Takato, T Strateva, IV Crawford, JL Ianna, PA McCarthy, DW Nelan, E Jefferys, WH van Altena, W Shelus, PJ Hemenway, PD Duncombe, RL Story, D Whipple, AL Bradley, AJ Fredrick, LW
Citation: Gf. Benedict et al., Precise masses for Wolf 1062 AB from Hubble Space Telescope interferometric astrometry and McDonald Observatory radial velocities, ASTRONOM J, 121(3), 2001, pp. 1607-1613
Interferometric astrometry of the low-mass binary Gl 791.2 (=HU Del) usingHubble Space Telescope fine guidance sensor 3: Parallax and component masses
Authors: Benedict, GF McArthur, BE Franz, OG Wasserman, LH Henry, TJ
Citation: Gf. Benedict et al., Interferometric astrometry of the low-mass binary Gl 791.2 (=HU Del) usingHubble Space Telescope fine guidance sensor 3: Parallax and component masses, ASTRONOM J, 120(2), 2000, pp. 1106-1112
Interferometric astrometry of the detached white dwarf-M dwarf binary Feige 24 using HST Fine Guidance Sensor 3: White dwarf radius and component mass estimates
Authors: Benedict, GF McArthur, BE Franz, OG Wasserman, LH Nelan, E Lee, J Fredrick, LW Jefferys, WH van Altena, W Robinson, EL Spiesman, WJ Shelus, PJ Hemenway, PD Duncombe, RL Story, D Whipple, AL Bradley, A
Citation: Gf. Benedict et al., Interferometric astrometry of the detached white dwarf-M dwarf binary Feige 24 using HST Fine Guidance Sensor 3: White dwarf radius and component mass estimates, ASTRONOM J, 119(5), 2000, pp. 2382-2390
Astrometry with Hubble Space Telescope Fine Guidance Sensor 3: The parallax of the cataclysmic variable RW Triangulum
Authors: McArthur, BE Benedict, GF Lee, J Lu, CL van Altena, WF Deliyannis, CP Girard, T Fredrick, LW Nelan, E Duncombe, RL Hemenway, PD Jefferys, WH Shelus, PJ Franz, OG Wasserman, LH
Citation: Be. Mcarthur et al., Astrometry with Hubble Space Telescope Fine Guidance Sensor 3: The parallax of the cataclysmic variable RW Triangulum, ASTROPHYS J, 520(1), 1999, pp. L59-L62
Hubble Space Telescope Fine Guidance Sensor astrometric parallaxes for three dwarf novae: SS Aurigae, SS Cygni, and U Geminorum
Authors: Harrison, TE McNamara, BJ Szkody, P McArthur, BE Benedict, GF Klemola, AR Gilliland, RL
Citation: Te. Harrison et al., Hubble Space Telescope Fine Guidance Sensor astrometric parallaxes for three dwarf novae: SS Aurigae, SS Cygni, and U Geminorum, ASTROPHYS J, 515(2), 1999, pp. L93-L96
The optical mass-luminosity relation at the end of the main sequence (0.08-0.20 M-circle dot)
Authors: Henry, TJ Franz, OG Wasserman, LH Benedict, GF Shelus, PJ Ianna, PA Kirkpatrick, JD McCarthy, DW
Citation: Tj. Henry et al., The optical mass-luminosity relation at the end of the main sequence (0.08-0.20 M-circle dot), ASTROPHYS J, 512(2), 1999, pp. 864-873
Interferometric astrometry of Proxima Centauri and Barnard's star using Hubble Space Telescope Fine Guidance Sensor 3: Detection limits for substellar companions
Authors: Benedict, GF McArthur, B Chappell, DW Nelan, E Jefferys, WH van Altena, W Lee, J Cornell, D Shelus, PJ Hemenway, PD Franz, OG Wasserman, LH Duncombe, RL Story, D Whipple, AL Fredrick, LW
Citation: Gf. Benedict et al., Interferometric astrometry of Proxima Centauri and Barnard's star using Hubble Space Telescope Fine Guidance Sensor 3: Detection limits for substellar companions, ASTRONOM J, 118(2), 1999, pp. 1086-1100
Risultati: 1-8 |