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 11084


Contents

Images

Upload your image

DSS Images   Other Images


Related articles

Oxygen abundances in halo giants. I - Giants in the very metal-poor globular clusters M92 and M15 and the metal-poor halo field
Oxygen, iron, vanadium, and scandium abundances are derived for verymetal-poor giants in the globular clusters M92 and M15, and giants ofcomparable metallicity in the local halo field. The forbidden O I linedublet (6300, 6363) and nearby metallic lines in spectra are analyzedusing line analysis and spectral synthesis codes. The Fe/H abundance forM92 is estimated at -2.25 +/-0.02 based on nine giants with a range of500 K in effective temperature. No evidence for star-to-star variationsin the Fe/H abundance was found. O-rich and O-poor stars appearintermixed in the H-R diagram. O - N nuclear synthesis and mixing to thesurface are proposed as the best explanation for the low-oxygen giants.The nitrogen abundances obtained earlier for nine of the ten halo fieldgiants in this sample are incompatible with the very large nitrogenabundances expected of the O/Fe abundance of about + 1.2 in halo fieldsubdwarfs, as found by Abia and Rebolo (1989), and not more than 0.6 inhalo giants, as found in this and other studies.

Positional reference stars in the Magellanic Clouds
The equatorial coordinates are determined of 926 stars (mainly ofgalactic origin) in the direction of the Magellanic Clouds at the meanepoch T = 1978.4 with an overall accuracy characterized by the meanvalues of the O-C coordinates, Sa = 0.35 arcsec and Sd = 0.38 arcsec,calculated from the coordinates of the Perth reference stars. Thesevalues are larger than the accuracy expected for primary standard stars.They allow the new positions to be considered as those of reliablesecondary standard stars. The published positions correspond to anunquestionable improvement of the quality of the coordinates provided inthe current catalogs. This study represents an 'astrometric step' in thestarting of a 'Durchmusterung' of the Magellanic Clouds organized by deBoer (1988, 1989).

Submit a new article


Related links

  • - No Links Found -
Submit a new link


Member of following groups:


Observation and Astrometry data

Constellation:Hydrus
Right ascension:01h45m57.89s
Declination:-71°38'39.9"
Apparent magnitude:8.777
Distance:335.57 parsecs
Proper motion RA:13.6
Proper motion Dec:-5.3
B-T magnitude:10.285
V-T magnitude:8.902

Catalogs and designations:
Proper Names
HD 1989HD 11084
TYCHO-2 2000TYC 9146-596-1
USNO-A2.0USNO-A2 0150-01138638
HIPHIP 8228

→ Request more catalogs and designations from VizieR