关注
Douglas R. Gies
Douglas R. Gies
在 chara.gsu.edu 的电子邮件经过验证
标题
引用次数
引用次数
年份
A survey of stellar families: multiplicity of solar-type stars
D Raghavan, HA McAlister, TJ Henry, DW Latham, GW Marcy, BD Mason, ...
The Astrophysical Journal Supplement Series 190 (1), 1, 2010
19732010
Carbon, nitrogen, and oxygen abundances in early B-type stars
DR Gies, DL Lambert
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 387, March 10, 1992, p …, 1992
5901992
ICCD speckle observations of binary stars. XIX. An astrometric/spectroscopic survey of O stars
BD Mason, DR Gies, WI Hartkopf, WG Bagnuolo Jr, T Ten Brummelaar, ...
The Astronomical Journal 115 (2), 821, 1998
5361998
The binary frequency and origin of the OB runaway stars
DR Gies, CT Bolton
Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 61, June 1986 …, 1986
4671986
The high angular resolution multiplicity of massive stars
BD Mason, WI Hartkopf, DR Gies, TJ Henry, JW Helsel
The Astronomical Journal 137 (2), 3358, 2009
4472009
The kinematical and binary properties of association and field O stars
DR Gies
Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 64, July 1987 …, 1987
3871987
The optical spectrum of HDE 226868= Cygnus X-1. II Spectrophotometry and mass estimates.
DR Gies, CT Bolton
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 304, May 1, 1986, p …, 1986
3511986
ABSORPTION LINE PROFILE VARIATIONS AMONG THE O STARS. I. THE INCIDENCE OF VARIABILITY
AW Fulllerton, DR Gies, CT Bolton
Astrophysical Journal-Supplement Series only-Paper Edition 103 (2), 475-512, 1996
3091996
A stellar rotation census of B stars: from ZAMS to TAMS
W Huang, DR Gies, MV McSwain
The Astrophysical Journal 722 (1), 605, 2010
2632010
Stellar diameters and temperatures. III. Main-sequence A, F, G, and K stars: additional high-precision measurements and empirical relations
TS Boyajian, K Von Braun, G Van Belle, C Farrington, G Schaefer, ...
The Astrophysical Journal 771 (1), 40, 2013
2522013
Stellar diameters and temperatures. I. Main-sequence A, F, and G stars
TS Boyajian, HA McAlister, G Van Belle, DR Gies, TA Ten Brummelaar, ...
The Astrophysical Journal 746 (1), 101, 2012
2422012
The evolutionary status of Be stars: results from a photometric study of southern open clusters
MV McSwain, DR Gies
The Astrophysical Journal Supplement Series 161 (1), 118, 2005
2362005
First results from the CHARA array. I. An interferometric and spectroscopic study of the fast rotator α Leonis (Regulus)
HA McAlister, TA Ten Brummelaar, DR Gies, W Huang, WG Bagnuolo Jr, ...
The Astrophysical Journal 628 (1), 439, 2005
2252005
First results from the CHARA Array. IV. The interferometric radii of low-mass stars
DH Berger, DR Gies, HA McAlister, TA ten Brummelaar, TJ Henry, ...
The Astrophysical Journal 644 (1), 475, 2006
2082006
The line profile variations of Epsilon Persei. I-Evidence for multimode nonradial pulsations
DR Gies, A Kullavanijaya
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 326, March 15, 1988, p …, 1988
1961988
Coordinated ultraviolet and Halpha spectroscopy of bright O-type stars.
L Kaper, HF Henrichs, AW Fullerton, H Ando, KS Bjorkman, DR Gies, ...
Astronomy and Astrophysics, v. 327, p. 281-298 327, 281-298, 1997
1901997
Stellar rotation in young clusters. I. Evolution of projected rotational velocity distributions
W Huang, DR Gies
The Astrophysical Journal 648 (1), 580, 2006
1792006
Tomographic separation of composite spectra-The components of the O-star spectroscopic binary AO Cassiopeiae
WG Bagnuolo Jr, DR Gies
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 376, July 20, 1991, p …, 1991
1741991
Hubble space telescope Goddard high resolution spectrograph observations of the Be+ sdO binary ϕ Persei
DR Gies, WG Bagnuolo Jr, EC Ferrara, AB Kaye, ML Thaller, LR Penny, ...
The Astrophysical Journal 493 (1), 440, 1998
1631998
Stellar diameters and temperatures–V. 11 newly characterized exoplanet host stars
K Von Braun, TS Boyajian, GT van Belle, SR Kane, J Jones, C Farrington, ...
Monthly Notices of the Royal Astronomical Society 438 (3), 2413-2425, 2014
1562014
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