• Cowley Ch., Sheminova V.A.,Abundance sensitive points of line profiles in the stellar spectra. 2014,MNRAS,Vol.443,Is.3,p.1967-1972. 2014MNRAS.443.1967S
  • Khomenko E.V., Vitas N., Collados M., et al.Three-dimensional simulations of solar magneto- convection including effects of partial ionization. 2018,A&A,Vol.618,p.A87. 2018A&A...618A..87K
  • Shukirgaliyev B., Parmentier G., Just A., et al.The Long-term Evolution of Star Clusters Formed with a Centrally Peaked Star Formation Efficiency Profile. 2018,ApJ,Vol.863,p.171 (13 pp.). 2018ApJ...863..171S

 

 

 

 

Random photo

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Contacts

Reception:

Kuchmiy Hanna

tel.:
fax:
internal address:

+(380) 44 526-31-10
+(380) 44 526-21-47
room 207, tel. 3-55

 

Office:

Head clerk Korsun Tetiana

tel.:
fax:
internal address:

+(380) 44 526-08-69
+(380) 44 526-21-47
office(at)mao.kiev.ua
room 230, tel. 3-57

 

Postal address:

Main astronomical observatory

of National academy of sciences of Ukraine

27 Akademika Zabolotnoho St.

03143,Kyiv, Ukraine

 

Transit:
trolleybus №11 ( from Expotsentr (The National Complex “Expocenter of Ukraine”)stop to the last stop)
or minibus №496 (from Lukianivska metro station or bus stops "Epitsentr", "Zabolotnoho", "Metrologichna" to the stop: "Feofania hospital, housing 2").



MAO on the Google Maps