Home     To Survive in the Universe    
Services
    Why to Inhabit     Top Contributors     Astro Photo     The Collection     Forum     Blog New!     FAQ     Login  
→ Adopt this star  

HD 20061


Contents

Images

Upload your image

DSS Images   Other Images


Related articles

uvby - β Photoelectric Photometry of the Open Cluster α Per
Absolute photoelectric photometry of stars in the direction of the OpenCluster α Per has been secured and is presented along with ananalysis reinforced with all the available data in Strömgrenuvby-β photometry compiled from the literature. Cluster membershipis analyzed and the physical characteristics of the stars have beendeduced. The membership determined in this paper is compared with thatof proper motion studies and Hipparcos.

Analysis of IRAS stellar sources in Alpha Persei region
The present study is an analysis of IR sources in the Alpha Persei opencluster region from the IRAS Point Source Catalog and from ground-basedphotometric observations. Cross-identification between stars in theregion and IRAS Point Source Catalog was performed and nine newassociations were found. BVRI Johnson photometry for 24 of the matchedobjects have been carried out. Physical identity of visual and IRASsources and relationship to the Alpha Persei open cluster are discussed.

Membership of low-mass stars in the open cluster Alpha Persei
The results of a combined astrometric, photometric, and spectroscopicsearch for low-mass members in the intermediate-age open cluster AlphaPersei are presented. Over 130 low-mass new members have been identifiedto M(v) about 12.5, almost doubling the previous number of knownmembers. The new membership information suggests a slight upwardrevision of Alpha Per's age to about 8 x 10 exp 7 yr. Alpha Per isnoticeably spatially elongated in a direction parallel to the Galacticplane, most likely due to tidal deformation. Analysis of thedistribution of relative H-alpha emission strengths among Alpha Permembers confirms the view that the mean H-alpha strength decreases inincreasingly older systems. Allowing for survey incompleteness, onecannot reject the idea that the luminosity function is consistent withthe field luminosity function to M(v) about 9 or 10.

Uvby-Beta Photometry for 67 Stars in the Region of Alpha-Persei
Abstract image available at:http://adsabs.harvard.edu/abs/1989A&AS...81...47T

Measurements of 258 radial velocities in two fields near Alpha Per
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1987A&AS...68..515F&db_key=AST

On the relationship between the apparent magnitudes given in several catalogues and the UBV system.
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1974A&AS...15..215O&db_key=AST

Eigenbewegungen in der Umgebung von α Persei
Not Available

Submit a new article


Related links

  • - No Links Found -
Submit a new link


Member of following groups:


Observation and Astrometry data

Constellation:ペルセウス座
Right ascension:03h15m31.49s
Declination:+50°55'32.7"
Apparent magnitude:8.446
Distance:476.19 parsecs
Proper motion RA:16.1
Proper motion Dec:-4.8
B-T magnitude:10.456
V-T magnitude:8.612

Catalogs and designations:
Proper Names
HD 1989HD 20061
TYCHO-2 2000TYC 3323-688-1
USNO-A2.0USNO-A2 1350-03219555
HIPHIP 15171

→ Request more catalogs and designations from VizieR