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מאמרים קשורים
Pulkovo compilation of radial velocities for 35495 stars in a common system.
Not Available
| 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
| Infrared carbon stars: new identifications and their space distribution in the Galaxy
We present JHKL photometry of a sample of 150 IRAS stars in the thirdand fourth galactic quadrant with | b | <2(deg) selected according totheir IRAS colour (0.160<=[12-25]<=1.156). We identify 27 carbonstar candidates using the [12-25] vs. K-L two-colour diagram method.Among them, 10 are listed in the Stephenson's catalogue of carbon starsand 17 are new infrared carbon stars (IRCS) candidates. Their distancesare found to be larger than 3 kpc. These data are combined with previousdata to study the space distribution of IRCS. The number density seemsto be independent of the galactocentric distance (R) toward the GalacticCenter and to decrease exponentially toward the anticenter. At thepresent stage, it is not possible to disentangle effects such asincompleteness of the sample, different space distribution law anddependence of the luminosity on metallicity. In particular, we suggestthat the apparent scarcity of IRCS in the central direction of theGalaxy (R<5 kpc) might be due to a selection effect. From theavailable data, we have found no IRCS within 1 kpc of the GalacticCenter. Based on observations obtained at the European SouthernObservatory, Chile
| Infrared Surveys of the Southern Milky way. II. Suspected Supergiant M Stars
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1972ApJ...176..623A&db_key=AST
| Spectroscopic and Photometric Observations of M Supergiants in Carina.
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1972ApJ...172...75H&db_key=AST
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משמש של הקבוצה הבאה
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תצפית ומידע אסטרומטרי
| קבוצת-כוכבים: | שדרית |
| התרוממות ימנית: | 10h36m11.97s |
| סירוב: | -57°51'46.5" |
| גודל גלוי: | 7.75 |
| מרחק: | 16666.667 פארסק |
| תנועה נכונה: | -7.4 |
| תנועה נכונה: | 2.6 |
| B-T magnitude: | 10.111 |
| V-T magnitude: | 7.945 |
קטלוגים וכינוים:
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