Contenuti
Immagini
Carica la tua immagine
DSS Images Other Images
Articoli relazionati
Hipparcos red stars in the HpV_T2 and V I_C systems
For Hipparcos M, S, and C spectral type stars, we provide calibratedinstantaneous (epoch) Cousins V - I color indices using newly derivedHpV_T2 photometry. Three new sets of ground-based Cousins V I data havebeen obtained for more than 170 carbon and red M giants. These datasetsin combination with the published sources of V I photometry served toobtain the calibration curves linking Hipparcos/Tycho Hp-V_T2 with theCousins V - I index. In total, 321 carbon stars and 4464 M- and S-typestars have new V - I indices. The standard error of the mean V - I isabout 0.1 mag or better down to Hp~9 although it deteriorates rapidly atfainter magnitudes. These V - I indices can be used to verify thepublished Hipparcos V - I color indices. Thus, we have identified ahandful of new cases where, instead of the real target, a random fieldstar has been observed. A considerable fraction of the DMSA/C and DMSA/Vsolutions for red stars appear not to be warranted. Most likely suchspurious solutions may originate from usage of a heavily biased color inthe astrometric processing.Based on observations from the Hipparcos astrometric satellite operatedby the European Space Agency (ESA 1997).}\fnmsep\thanks{Table 7 is onlyavailable in electronic form at the CDS via anonymous ftp tocdsarc.u-strasbg.fr (130.79.128.5) or viahttp://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/397/997
| The kinematics of the Small Magellanic Cloud from its field carbon stars
The present velocity survey observed 150 carbon stars in the SMC in thenear-IR with an individual precision of + or - 1.8 km/sec. Carbon starsare found to behave kinematically like the planetary nebulae system withwhich they share a velocity dispersion of about 27 km/sec; they alsoexhibit the same velocity dispersion as a sample of halo metal-poorgiants near NGC 121. The carbon stars and planetary nebulae may belongto a spheroidal system, and indications are found of streaming motionsin the wing section between the SMC and LMC.
|
Sottometti un nuovo articolo
Link relazionati
Sottometti un nuovo link
Membro dei seguenti gruppi:
|
Osservazione e dati astrometrici
| Costellazione: | Lince |
| Ascensione retta: | 07h29m14.94s |
| Declinazione: | +54°05'15.7" |
| Magnitudine apparente: | 9.642 |
| Moto proprio RA: | 1.2 |
| Moto proprio Dec: | 0.1 |
| B-T magnitude: | 11.864 |
| V-T magnitude: | 9.826 |
Cataloghi e designazioni:
|
