Clayton, G. C. |
Volume |
Paper Title |
Page Number |
Authors |
26 |
Dust Formation; Chromospheres in R Coronae Borealis Stars: How Where; Why? |
481 |
Clayton, G. C.; Whitney, B. A.; Stanford, S. A. |
45 |
Dust Formation in R-Coronae Stars |
115 |
Whitney, B. A.; Balm, S. P.; Clayton, G. C. |
83 |
Pulsations and Dust Formation in R Coronae Borealis Stars |
433 |
Clayton, G. C.; Whitney, B. A.; Lawson, W. A. |
97 |
Of Scattering Properties and Approximation Techniques: To EMT or Not To EMT |
48 |
Wolff, M. J.; Gibson, S. J.; Clayton, G. C. |
97 |
Astro-2 Observations of Ultraviolet Polarization and Extinction by Interstellar Dust in the LMC |
612 |
Green, J.; Clayton, G. C.; Wolff, M. J.; Zellner, N. E. B.; Code, A. D.; Davidsen, A. F.; The WUPPE Team; HUT Team |
97 |
Polarimetry of the Interstellar Medium: Concluding Summary |
618 |
Clayton, G. C. |
137 |
Polarimetry and Spectroscopy of the LMC X-Ray Binary A0538-66 |
454 |
Misselt, K. A.; Clayton, G. C.; Schulte-Ladbeck, R. E. |
168 |
Is the Extended Red Emission Due to CO? |
231 |
Bennett, P. D.; Harper, G. M.; Brown, A.; Clayton, G. C. |
193 |
Dust in High Redshift Starburst Galaxies |
517 |
Gordon, K. D.; Smith, T. L.; Clayton, G. C. |
196 |
Interpretation of Extragalactic Extinction Measurements Using the Maximum Entropy Method |
41 |
Clayton, G. C.; Wolff, M. J.; Gordon, K. D.; Misselt, K. A. |
203 |
New R Coronae Borealis Stars in the LMC Discovered in the MACHO Photometry Database |
114 |
Clayton, G. C.; Kilkenny, D.; Welch, D. L.; The MACHO Collaboration |
469 |
Are the R Coronae Borealis Stars Produced by White Dwarf Mergers? |
133 |
Clayton, G. C. |
469 |
Simulations of White Dwarf Mergers |
137 |
Staff, J.; Menon, A.; Herwig, F.; Clayton, G. C.; Even, W. P.; Fryer, C. L.; Motl, P.; Tohline, J. E.; Geballe, T.; Pignatari, M. |