Irregular eruptive variables
IN -
Orion variables. Irregular, eruptive variables connected with
bright or dark diffuse nebulae or observed in the regions of these
nebulae. Some of them may show cyclic light variations caused by
axial rotation. In the Spectrum-Luminosity diagram, they are
found in the area of the main sequence and subgiants. They are
probably young objects that, during the course of further
evolution, will become light-constant stars on the zero-age main
sequence (ZAMS). The range of brightness variations may reach
several magnitudes. In the case of rapid light variations having
been observed (up to 1 mag in 1-10 days), the letter "S" is added
to the symbol for the type (INS). This type may be divided into
the following subtypes:
- INA - Orion variables of early spectral types (B-A or Ae). They are often
characterized by occasional abrupt Algol-like fadings (T Ori);
- INB - Orion variables of intermediate and late spectral types, F-M or
Fe-Me (BH Cep, AH Ori). F-type stars may show Algol-like fadings
similar to those of many INA stars; K-M stars may produce flares
along with irregular light variations;
- INT,IT - Orion variables of the T Tauri type. Stars are assigned to
this type on the basis of the following (purely spectroscopic)
criteria: spectral types are in the range Fe-Me. The spectra of
most typical stars resemble the spectrum of the solar
chromosphere. The feature specific to the type is the presence of
the flourescent emission lines Fe II 4046, 4132 A (anomalously
intense in the spectra of these stars), emission lines [Si II] and
[O I], as well as the absorption line Li I 6707 A. These variables
are usually observed only in diffuse nebulae. If it is not
apparent that the star is associated with a nebula, the letter "N"
in the symbol for the type may be omitted, e.g., IT (RW AUR);
- IN(YY) - Some Orion variables (YY Ori) show the presence of absorption
components on the redward sides of emission lines, indicating the
infall of matter toward the stars' surfaces. In such cases, the
symbol for the type may be accompanied by the symbol "YY".
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