he interest for this class of variable %stars has significantly increased during the last decade and about %30 members are presently known in the literature. A new observational study of the Herbig Ae star VV Ser has been performed in order to detect and a

Details he interest for this class of variable %stars has significantly increased during the last decade and about %30 members are presently known in the literature. A new observational study of the Herbig Ae star VV Ser has been performed in order to detect and a he interest for this class of variable %stars has significantly increased during the last decade and about %30 members are presently known in the literature. A new observational study of the Herbig Ae star VV Ser has been performed in order to detect and a

Jan 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007waas.work...65r&link_type=abstract

"1st Workshop of Astronomy and Astrophysics for Students" held in Naples (ITALY) on April 19-20, 2006. Published by INFN-Naples,

Astronomy and Astrophysics

Astrophysics

Scientific paper

The study of pulsation in Pre-Main-Sequence (PMS) intermediate mass
stars represents an important tool to derive information on the stellar
parameters and structure, as well as to test the validity of current
theoretical models.

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