Főoldal     Alapinformációk     To Survive in the Universe    
Inhabited Sky
    News@Sky     Asztrofotók     Kollekció     Fórum     Blog New!     GYIK     Sajtó     Bejelentkezés  

HD 91669


Tartalom

Képek

Kép feltöltése

DSS Images   Other Images


Kapcsolódó cikkek

HD 91669B: A New Brown Dwarf Candidate from the McDonald Observatory Planet Search
We report the detection of a brown dwarf candidate orbiting themetal-rich K dwarf HD 91669, based on radial-velocity data from theMcDonald Observatory Planet Search. HD 91669b is a substellar object inan eccentric orbit (e = 0.45) at a separation of 1.2 AU. The minimummass of 30.6M Jup places this object firmly within the browndwarf desert for inclinations i gsim 23°. This is the second rareclose-in brown dwarf candidate discovered by the McDonald planet searchprogram.

Improved Astrometry and Photometry for the Luyten Catalog. II. Faint Stars and the Revised Catalog
We complete construction of a catalog containing improved astrometry andnew optical/infrared photometry for the vast majority of NLTT starslying in the overlap of regions covered by POSS I and by the secondincremental Two Micron All Sky Survey (2MASS) release, approximately 44%of the sky. The epoch 2000 positions are typically accurate to 130 mas,the proper motions to 5.5 mas yr-1, and the V-J colors to0.25 mag. Relative proper motions of binary components are measured to 3mas yr-1. The false-identification rate is ~1% for11<~V<~18 and substantially less at brighter magnitudes. Theseimprovements permit the construction of a reduced proper-motion diagramthat, for the first time, allows one to classify NLTT stars intomain-sequence (MS) stars, subdwarfs (SDs), and white dwarfs (WDs). We inturn use this diagram to analyze the properties of both our catalog andthe NLTT catalog on which it is based. In sharp contrast to popularbelief, we find that NLTT incompleteness in the plane is almostcompletely concentrated in MS stars, and that SDs and WDs are detectedalmost uniformly over the sky δ>-33deg. Our catalogwill therefore provide a powerful tool to probe these populationsstatistically, as well as to reliably identify individual SDs and WDs.

Structure and motions in the CAR spiral feature.
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1972A&A....20...29H&db_key=AST

Új cikk hozzáadása


Kapcsolódó hivatkozások

  • - (nincs kapcsolódó hivatkozás) -
Új link hozzáadása


Besorolás csoportokba:


Pozíciós és asztrometriai adatok

Csillagkép:Északi Vízikígyó
Rektaszcenzió:10h34m54.43s
Deklináció:-13°47'16.6"
Vizuális fényesség:9.705
RA sajátmozgás:116
Dec sajátmozgás:-176.5
B-T magnitude:10.853
V-T magnitude:9.8

Katalógusok és elnevezések:
Megfelelő nevek   (Edit)
HD 1989HD 91669
TYCHO-2 2000TYC 5498-683-1
USNO-A2.0USNO-A2 0750-07292462
HIPHIP 51789

→ További katalógusok és elnevezések lekérése VizieR-ből