V0380 Cephei
catalogues and names |
SKY2000 - Master Star Catalog |
Smithsonian Astrophysical Observatory Star Catalog |
Combined General Catalogue of Variable Stars (Vol. I-III) |
catalogues and names
catalogues and names | V0380 Cep, HD 200775, SAO 19158, BD +67 1283 |
data from SKY2000 - Master Star Catalog (Myers+ 1997)
position, motion, parallax:
position (J2000) | RA: 21h 1min 36.94sec | DEC: +68° 9' 47.87'' | ±0.2 arcsec | source: 15 |
position (2000.74) | RA: 21h 1min 38sec | DEC: +68° 9' 58'' | JD: 2451813.20 | |
proper motion (J2000) | RA: 0.0015 arcsec/a | DEC: -0.002 arcsec/a | source: 15 | |
radial velocity | -3.3 km/s | source: 15 | ||
galactic coord. (B1950) | longitude: 104.06° | latitude: 14.19° |
magnitude:
visual | 7.36 (observed) | source: 20 |
photovisual | 7.2 | source: 2 |
photographic | 7.5 | source: 16 |
spectral information:
spectral class | B5 | source: 96 | |
Morgan-Keenan | B2V | source: 98 | |
B-magnitude | 7.74 ±0.011 | B-V-magnitude | 0.38 |
U-magnitude | 7.35 ±0.007 | U-B-magnitude | -0.39 |
sources:
2 | HD and HDE Catalogs |
Cannon, A.J., and E.C. Pickering, Harvard Annals, Vols 91-99, 1918-24, Cambridge, Massachusetts: Harvard University; Cannon, A.J., Harvard Annals, Vol. 100, 1925-36, Cambridge, Massachusetts: Harvard University; and Cannon, A.J., and M. Walton Mayall, Harvard Annals, Vol. 112, 1949, Cambridge, Massachusetts: Harvard University | |
15 | FK5, FK5 Extension and FK5 Supplement |
Fricke, W., H. Schwan and T. Lederle, "Fifth Fundamental Catalogue (FK5), Part I. The Basic Fundamental Stars," Veroff. Astronomisches Recheninstitut, No. 32, Heidelberg, Germany, 1988, and Fricke, W., H. Schwan, and T.E. Corbin, "Fifth Fundamental Catalogue (FK5), Part II. The FK5 Extension," Veröff. Astronomisches Recheninstitut, No. 33, Heidelberg, Germany, 1991 | |
16 | PPM North and PPM South Catalogs and PPM Supplement |
Roser, S., and U. Bastian, "Catalogue of Positions and Proper Motions," A&AS, Vol. 74, p. 449, 1988, and Bastian, U., et al., "Catalogue of Positions and Proper Motions - South," 1993 | |
20 | Catalogue of Homogeneous Means in the UBV System |
Mermilliod, J.C., Catalogue of Homogeneous Means in the UBV System, Institut d'Astronomie, Universite de Lausanne, 1994 | |
96 | SAO or HD/HDE Catalog |
Reference from Value 1 or Reference from Value 2 | |
98 | SKYMAP Master Catalog Version 3.7 |
Reference from Value 97 [original data sources Catalog Version 3.7 are identified in SKYMAP Version 3.7] |
data from Smithsonian Astrophysical Observatory Star Catalog (SAO Staff 1966; USNO, ADC 1990)
position and proper motion:
position (B1950) | RA: 21h 0min 59.7sec | DEC: +67° 57' 55.5'' | ±0.032 arcsec |
position (2000.74) | RA: 21h 1min 38sec | DEC: +68° 9' 58'' | JD: 2451813.20 |
position (J2000) | RA: 21h 1min 36.933sec | DEC: +68° 9' 48.3'' | |
proper motion B1950 (FK4) | RA: 0.001 arcsec/a | DEC: 0.01 arcsec/a | ±0.007 arcsec/a in RA ±0.009 arcsec/a in DEC |
proper motion J2000 (FK5) | RA: 0.0014 arcsec/a | DEC: 0.006 arcsec/a | |
source of proper motion data | Determined by source catalog |
magnitude:
visual | 7.2 (accuracy: 2 decimals) |
source of visual magnitude data | Taken from Harvard or San Luis photometry. |
spectral information:
spectral class | B5 |
source of spectral data | Taken from the Henry Draper Catalogue or no spectrum in source catalog. |
catalogues
source catalogue | GC, catalogue number: 29401 |
Durchmusterung | BD+67 1283 |
Boss General Catalogue | 29401 |
Henry Draper Catalogue | 200775 |
data from Combined General Catalogue of Variable Stars (Vol. I-III) (Kholopov+ 1998)
position:
position (equinox 1950.0) | RA: 21h 0min 59.7sec | DEC: +67° 57' 56'' |
variability informations:
variability type | INA | eruptive variable star |
magnitute at max. brightness | 7.1 | |
magnitute at min. brightness | 7.36 | |
photometric system |
references
to a study | Yu.K.Bergner, A.S.Miroshnichenko, R.V.Yudin, N.Yu.Yutanov, K.S.Kuratov, D.B. Mukanov, Astr Tsirk No.1396, 1, 1985. |
to a chart/photograph | V.S.Shevchenko, M.A.Ibragimov, S.D.Yakubov, Soviet Astronomy 33, No.5, 487, 1989 = Astr Zh (USSR) 66, No.5, 941, 1989. |
miscanellous
ID in the GCVS catalogue | 20/380 |
constellation | Cepheus |
notes on existence | The star is equivalent to '72470'. |
variability type description
variability type | description |
INA | 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, INB, INT, IN(YY). 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 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". |