NNo GCVS J2000.0 Type Max Min I Min II Epoch Year Period M-m/D Spectrum References Other desig. p.m.(as/yr) Epoch Ident. New type GCVS -------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------- 639002 |bet Per *|030810.13 +405720.4 |EA/SD | 2.12 | 3.39 | |V |45641.5135 | | 2.8673043 |14 *|B8V |00001 08953| |+0.002 -0.001|2000.0 | |Hip | |bet Per | -------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------- _______________Cross-identifications:_______________ bet Per = ADS 02362 |A bet Per = BAY Per bet | bet Per = BD +40 0673 | bet Per = BS 00936 | bet Per = CRL 0443 | bet Per = FLM Per 026 | bet Per = GSC 02851.02168 | bet Per = HD 019356 | bet Per = Hip 014576 | bet Per = IRAS 03048+4045 | bet Per = IRC +40055 | bet Per = SAO 038592 | bet Per = X 03049+407 | ____________________________________________________ Reference to a chart or photograph:
08953. AAVSO Variable Star Atlas, 1980.Reference to a study of the star:
00001. GCVS compilers.__________________________________________________________________
Remark: Multiple system (Eclipsing pair = Algol AB; Algol C 4.7m, Am, a = 0".10, Porb = 1.862a); Algol AB = ADS 2362 A (B 12.7m, 57".5, 156deg, 1920). P var. P = 2.8673442d (1784 - 1835); P = 2.8673012d (1835 - 1854); P = 2.8672775d (1854 - 1901); P = 2.8672967d (1901 - 1913); P = 2.8672506d (1913 - 1915) [06156]; Min I = 2424477.806 + 2.86730236d*E (JD2420500 - 25000); Min = 2425917.203 + 2.86732697d*E (JD2425000 - 277000); Min I = 2433194.454 + 2.86731667d*E (JD2427700 - 33600); Min I = 2433928.4944 + 2.86732442d*E (JD2433600 - 37000); Min I = 2437598.6766 + 2.86733732d*E (JD2437000 - 42200); since JD2442200 - see Table. Porb (Algol C) = 1.862a may be traced in the deviations; a period of 32a may also be real. Depth of Min I var. Variable polarization, changes in hydrogen line profiles, sometimes emissions in the spectrum. Radio source with frequent burst of different amplitude, faint X-ray source.
----The End----