בית     התחל מכאן     To Survive in the Universe    
Inhabited Sky
    News@Sky     תמונת אסטרו     האוסף     קבוצת דיון     Blog New!     שאלות נפוצות     עיתונות     כניסה  

HD 233392


תוכן

תמונות

הוסף תמונה שלך

DSS Images   Other Images


מאמרים קשורים

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.

הכנס מאמר חדש


לינקים קשורים

  • - לא נמצאו לינקים -
הכנס לינק חדש


משמש של הקבוצה הבאה


תצפית ומידע אסטרומטרי

קבוצת-כוכבים:לינכס
התרוממות ימנית:07h29m14.94s
סירוב:+54°05'15.7"
גודל גלוי:9.642
תנועה נכונה:1.2
תנועה נכונה:0.1
B-T magnitude:11.864
V-T magnitude:9.826

קטלוגים וכינוים:
שם עצם פרטי   (Edit)
HD 1989HD 233392
TYCHO-2 2000TYC 3781-879-1
USNO-A2.0USNO-A2 1425-06941981
HIPHIP 36380

→ הזמן עוד קטלוגים וכינוים מוזיר