Scale Height of Mira Variables

Autor(en)
Z. Berend, Josef Hron, Lajos G. Balazs, Franz Kerschbaum
Abstrakt

We estimated the scale height of intermediate and short period Miras making use of the maximum likelihood method. The available sample contains 1394 Mira variables. We divided these variables according to their periods. Our selection criterion was: |b| > 30deg because the interstellar absorption is practically negligible in this region at lambda = 12 micron. 85 intermediate period and 140 short period Miras have been left after the selection, their estimated scale heights are 260 pc and 590 pc respectively.

Organisation(en)
Institut für Astrophysik
Externe Organisation(en)
Hungarian Academy of Sciences
Journal
Communications from the Konkoly Observatory of the Hungarian Academy of Sciences
Band
100
Seiten
319
ISSN
0324-2234
Publikationsdatum
01-1997
ÖFOS 2012
103003 Astronomie, 103004 Astrophysik
Link zum Portal
https://ucrisportal.univie.ac.at/de/publications/scale-height-of-mira-variables(40cdb44d-53d8-4a04-b15a-307594c72cfc).html