Costas D. Papaliolios
Affiliations: | 1965-2001 | Physics | Harvard University, Cambridge, MA, United States |
Website:
http://news.harvard.edu/gazette/2002/07.18/24-papaliolios.htmlGoogle:
"Costas Demetrios Papaliolios"Bio:
https://books.google.nl/books?id=edMWAAAAYAAJ
http://adsabs.harvard.edu/abs/1965PhDT.........7P
Mean distance: 24.03 | S | N | B | C | P |
Parents
Sign in to add mentorNathaniel Phillips Carleton | grad student | 1965 | Harvard | |
(Excitation of metastable states of N2 and CO by electron impact.) |
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Publications
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Monnier JD, Traub WA, Schloerb FP, et al. (2004) First Results with the IOTA3 Imaging Interferometer: The Spectroscopic Binaries λ Virginis and WR 140 The Astrophysical Journal. 602 |
Marengo M, Karovska M, Sasselov DD, et al. (2003) Theoretical limb darkening for classical Cepheids. II. Corrections for the geometric Baade-Wesselink method Astrophysical Journal. 589: 968-975 |
Marengo M, Karovska M, Sasselov D, et al. (2003) Calibrating the Cepheid Period-Luminosity relation with the VLTI Eas Publications Series. 6: 265-265 |
Monnier JD, Berger JP, Millan-Gabet R, et al. (2002) SMART precision interferometry at 794 nm Proceedings of Spie - the International Society For Optical Engineering. 4838: 1127-1138 |
Marengo M, Sasselov DD, Karovska M, et al. (2002) Theoretical limb darkening for pulsating Cepheids Astrophysical Journal. 567: 1131-1139 |
Nisenson P, Papaliolios C. (2001) Detection of Earth-like Planets Using Apodized Telescopes The Astrophysical Journal. 548 |
Traub WA, Carleton NP, Bregman JD, et al. (2000) Third telescope project at the IOTA interferometer Astronomical Telescopes and Instrumentation. 4006: 715-722 |
Nisenson P, Papaliolios C. (1999) A Second Bright Source Detected near SN 1987A The Astrophysical Journal. 518 |
Coldwell CM, Papaliolios CD, Traub WA. (1998) First visible-light measurements from the IOTA interferometer Astronomical Telescopes and Instrumentation. 3350: 424-431 |
Karovska M, Nisenson P, Papaliolios C, et al. (1991) Asymmetries in the Atmosphere of Mira The Astrophysical Journal. 374 |