| Contents
 
 ImagesUpload your image
 DSS Images   Other Images
 
 
 
 Related articles
Submit a new article| Dwarfs in the Local Region We present lithium, carbon, and oxygen abundance data for a sample ofnearby dwarfs-a total of 216 stars-including samples within 15 pc of theSun, as well as a sample of local close giant planet (CGP) hosts (55stars) and comparison stars. The spectroscopic data for this work have aresolution of R~60,000, a signal-to-noise ratio >150, and spectralcoverage from 475 to 685 nm. We have redetermined parameters and derivedadditional abundances (Z>10) for the CGP host and comparison samples.From our abundances for elements with Z>6 we determine the meanabundance of all elements in the CGP hosts to range from 0.1 to 0.2 dexhigher than nonhosts. However, when relative abundances ([x/Fe]) areconsidered we detect no differences in the samples. We find nodifference in the lithium contents of the hosts versus the nonhosts. Theplanet hosts appear to be the metal-rich extension of local regionabundances, and overall trends in the abundances are dominated byGalactic chemical evolution. A consideration of the kinematics of thesample shows that the planet hosts are spread through velocity space;they are not exclusively stars of the thin disk.
 
 
 |  | Li-rich giants: A survey based on IRAS colours In a previous work we studied the IRAS colours of known Li-rich redgiants and showed that they have flux ratiosF12/F25 and F25/F60 in welldefined ranges. By using this result as a selection criterion, weprepared a list of 280 IRAS Point Source candidates to be Li-rich giantstars. Up to the present we have obtained spectra for 57% of our targetlist. We identified five stars showing a strong LiI 670.079 nm line andsix ones with a Li line of medium strength. Most of the candidates showfeatures typical of normal giants having circumstellar dust, asindicated by their IRAS colours. Observations collected at theLaboratorio Nacional de Astrofisica - LNA, Brazil; Observatoire de HauteProvence - OHP, France; European Southern Observatory - ESO, Chile.
 
 
 |  
 
 
 Related linksSubmit a new link
 
 
 Member of following groups: | 
 
 Observation and Astrometry data
| Constellation: | Orion |  | Right ascension: | 05h53m18.01s |  | Declination: | +09°33'32.0" |  | Apparent magnitude: | 7.225 |  | Distance: | 543.478 parsecs |  | Proper motion RA: | -25.1 |  | Proper motion Dec: | -13.6 |  | B-T magnitude: | 9.059 |  | V-T magnitude: | 7.377 |  Catalogs and designations:
 
 
 |