... flyby of Comet P/Honda-Mrhos-Pajdusakova on February 3, 1996 at about 21.00 GMT (approaching the nucleus along the tail) some 0.17 AU from the Sun , and a 14-million-kilometer (8.7-million-mile) passage of Comet P/Giacobini-Zinner on November 29, 1998 ...
23. http://www.arcetri.astro.it/tozzi/publ_ref.html
... Cremonese, G., Boehnhardt, H., Crovisier, J., Rauer, H., Fitzsimmons, A., Fulle, M., Licandro, J., Pollacco, D., Tozzi, G. P., & West, R. M. 1997, Astrophysical Journal Neutral Sodium from Comet Hale-Bopp: A Third Type of Tail . ...
24. Hypothetical Planets
... But Kowal suspected it may be very comet-like, and later it has even developed a short cometary tail. ...
25. Astrobigne 2014-2015
... Using a quasi 1-D approximation, we find that mass loading leads to the fast expansion of the pulsar wind tail, making the tail flow intrinsically non-stationary. ...
26. Astrobigne 2014-2015
... Using a quasi 1-D approximation, we find that mass loading leads to the fast expansion of the pulsar wind tail, making the tail flow intrinsically non-stationary. ...
27. Astrobigne 2014-2015
... Using a quasi 1-D approximation, we find that mass loading leads to the fast expansion of the pulsar wind tail, making the tail flow intrinsically non-stationary. ...
28. INAF - Osservatorio di Arcetri
... Using a quasi 1-D approximation, we find that mass loading leads to the fast expansion of the pulsar wind tail, making the tail flow intrinsically non-stationary. ...
29. INAF - Osservatorio di Arcetri
... Using a quasi 1-D approximation, we find that mass loading leads to the fast expansion of the pulsar wind tail, making the tail flow intrinsically non-stationary. ...
30. INAF - Osservatorio di Arcetri
... Using a quasi 1-D approximation, we find that mass loading leads to the fast expansion of the pulsar wind tail, making the tail flow intrinsically non-stationary. ...