✦ LIBER ✦

Striated features in the dust tail of comet C/2006 P1 (McNaught)

✍ Scribed by S. V. Kharchuk; P. P. Korsun

Book ID: 111498165
Publisher: Allerton Press Inc
Year: 2010
Tongue: English
Weight: 570 KB
Volume: 26
Category: Article
ISSN: 0884-5913
DOI: 10.3103/s0884591310060048

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

Inferior mirage of Comet McNaught (C/200

Inferior mirage of Comet McNaught (C/2006 P1)

✍ Mila Zinkova 📂 Article 📅 2011 🏛 John Wiley and Sons 🌐 English ⚖ 232 KB

Physical characteristics of the plasma t

Physical characteristics of the plasma tail of comet C/2009 R1 (McNaught)

✍ S. A. Borisenko, Yu. V. Sizonenko 📂 Article 📅 2012 🏛 Allerton Press Inc 🌐 English ⚖ 702 KB

Distribution Law For Particle Fragmentat

Distribution Law For Particle Fragmentation Times In A Theory For Striated Tails Of Dust Comets: Application To Comet Hale-Bopp (C/1995 O1)

✍ Z. Sekenina; J. Pittichová 📂 Article 📅 1997 🏛 Springer Netherlands 🌐 English ⚖ 66 KB

An Early Investigation Of The Striated T

An Early Investigation Of The Striated Tail Of Comet Hale-Bopp (C/1995 O1)

✍ J. Pittichovâ; Z. Sekenina; K. Birkle; J. Boehnhardt; D. Engels; P. Keller 📂 Article 📅 1997 🏛 Springer Netherlands 🌐 English ⚖ 85 KB

Infrared measurements of the chemical co

Infrared measurements of the chemical composition of C/2006 P1 McNaught

✍ Neil Dello Russo; Ronald J. Vervack Jr.; Harold A. Weaver; Carey M. Lisse 📂 Article 📅 2009 🏛 Elsevier Science 🌐 English ⚖ 770 KB

C/2006 P1 McNaught is a dynamically new comet from the Oort cloud that passed very close to the Sun, driving overall volatile production rates up to about 10 31 molecules s -1 . Post-perihelion observations were obtained in a target-of-opportunity campaign using the CSHELL instrument at the NASA Inf

Physical conditions in the plasma tail o

Physical conditions in the plasma tail of comet C/1987 P1 bradfield

✍ S. A. Borysenko; Yu. V. Sizonenko; I. V. Luk’yanyk; A. V. Ivanova; A. D. Voitsek 📂 Article 📅 2011 🏛 Allerton Press Inc 🌐 English ⚖ 681 KB