Poчetna     Да почнемо     To Survive in the Universe    
Inhabited Sky
    News@Sky     Астро Фотографије     Колекција     Форум     Blog New!     FAQ(Често постављана питања     Штампа     Улогуј се  

TYC 2002-987-1


Садржај

Слике

Уплоадјуј своје слике

DSS Images   Other Images


Везани чланци

Pulkovo compilation of radial velocities for 35495 stars in a common system.
Not Available

Kinematics and properties of F stars near the North Galactic Pole. II - The isothermal disc
Radial velocities are given for about 550 photometrically-identifieddisk-population F stars lying within 15 deg of the North Galactic Pole.The overall radial and z-velocity distributions are found to be closelyGaussian, with corrected rms and mean z velocities of 11.3 + or - 0.6and -9.5 + or - 0.5 km/s, respectively. The isothermal kinematics of thepopulation are reflected in the constant velocity dispersion to a zdistance of 400 pc. No systematic variation of either the velocitydispersion or the stellar age with the metallicity-sensitive Stromgrendelta m1 index is noted over a range of ages up to 5 Gyr.

Further Studies of A-Stars and F-Stars in the Region of the North Galactic Pole - Part Four - a Catalogue of Uvbyr Photometry and Derived Quantities
Not Available

Further Studies of A-Stars and F-Stars in the Region of the North Galactic Pole - Part Three - a Catalogue of Star Names and Positions
Not Available

Interstellar reddening near the north galactic pole
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1972PASP...84..497F&db_key=AST

Додај нови чланак


Линкови у сродству са темом

  • - Нема линкова -
Додај нови линк


Чланови следећих група \:

Посматрања и Астрометриски подаци

Сазвежђа:Волар
Ректацензија:13h52m31.09s
Deклинација:+25°01'39.0"
Apparent магнитуда:9.768
Proper motion RA:-6
Proper motion Dec:-3.4
B-T magnitude:10.201
V-T magnitude:9.804

Каталог и designations:
Proper имена   (Edit)
TYCHO-2 2000TYC 2002-987-1
USNO-A2.0USNO-A2 1125-06823160
HIPHIP 67733
→ Захтевај још каталога од VizieR