TOWARD UNDERSTANDING THE B[e] PHENOMENON. III. PROPERTIES OF THE OPTICAL COUNTERPART OF IRAS 00470+6429 Article (Web of Science)

Industry Collaboration International Collaboration

cited authors

  • Miroshnichenko, A. S.; Chentsov, E. L.; Klochkova, V. G.; Zharikov, S. V.; Grankin, K. N.; Kusakin, A. V.; Gandet, T. L.; Klingenberg, G.; Kildahl, S.; Rudy, R. J.; Lynch, D. K.; Venturini, C. C.; Mazuk, S.; Puetter, R. C.; Perry, R. B.; Carciofi, A. C.; Bjorkman, K. S.; Gray, R. O.; Bernabei, S.; Polcaro, V. F.; Viotti, R. F.; Norci, L.

publication date

  • July 20, 2009

webpage

published in

author keyword

  • circumstellar matter
  • stars: early-type
  • stars: emission-line, Be
  • stars: individual (IRAS 00470+6429)

category

start page

  • 209

end page

  • 220

volume

  • 700

issue

  • 1