Prohlížení Ústřední knihovna ČVUT dle autora "Nagashima, M."

Zobrazují se záznamy 1-3 z 3

    • Detection of Diatomic Molecules in the Dust Forming Nova V2676 Oph 

      Autor: Nagashima, M.; Arai, A.; Kajikawa, T.; Kawakita, H.; Kitao, E.; Arasaki, T.; Taguchi, G.; Ikeda, Y.
      (České vysoké učení technické v PrazeCzech Technical University in Prague, 2015)
      Novae are generally considered to be hot astronomical objects and show effective temperatures up to 10,000 K or higher at their visual maximum. But, it is theoretically predicted that the outer envelope of the nova outflow ...

    • Line Evolution of the Nova V5587 Sgr from Early to Nebula Phase 

      Autor: Kajikawa, T.; Arai, A.; Nagashima, M.; Kawakita, H.; Yamanaka, M.; Kawabata, K.; Kiyota, S.
      (České vysoké učení technické v PrazeCzech Technical University in Prague, 2015)
      The spectral evolution of the nova V5587 Sgr has been monitored at Koyama Astronomical Observatory and Higashi-Hiroshima Observatory, Japan, from the early to nebula phase. The nova rebrightened several times. The spectra ...

    • Spectroscopic Monitoring Observations of Nova V1724 Aql in 2012 

      Autor: Kajikawa, T.; Nagashima, M.; Kawakita, H.; Arai, A.; Ikeda, Y.; Isogai, M.; Fujii, M.; Ayani, K.
      (České vysoké učení technické v PrazeCzech Technical University in Prague, 2015)
      Spectroscopic and photometric monitoring observations of nova Apl 2012 (V1724 Apl) were conducted at Koyama Astronomical Observatory, Fujii-Kurosaki Observatory and Bisei Astronomical Observatory. The nova was initially ...