| Issue |
A&A
Volume 469, Number 2, July II 2007
|
|
|---|---|---|
| Page(s) | 771 - 776 | |
| Section | Planets and planetary systems | |
| DOI | https://doi.org/10.1051/0004-6361:20077286 | |
| Published online | 24 April 2007 | |
Photometry and imaging of comet C/2004 Q2 (Machholz) at Lulin and La Silla
1
Institute of Astronomy, National Central University, 300 Jungda Rd, Jungli City, Taiwan e-mail: s1249002@cc.ncu.edu.tw
2
Institut fur Planetenforschung, DLR, Rutherfordstr. 2, 12489 Berlin, Germany
Received:
13
February
2007
Accepted:
20
March
2007
Aims.We have investigated the development of the dust and gas coma of the comet C/2004 Q2 (Machholz) from December 2004 to January 2005 using observations obtained at the Lulin Observatory, Taiwan and the European Southern Observatory at La Silla, Chile.
Methods.We determined the dust-activity parameter 
and the dust color and derived Haser production
rates and scale lengths of 
and 
. An image enhancement technique was applied to
study the morphology of the gas and dust coma.
Results.Two jets were observed in the coma distributions of and CN of comet Machholz that
were not formed in the dust coma. The jets showed a spiral-like structure and pointed at different
position angles at different observing times. The formation of these jets can be explained by the
presence of two active surface regions on a rotating cometary nucleus.
Key words: comets: indvidual: C/2004Q2 (Machholz)
© ESO, 2007
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