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HD 75138


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A second list of wide visual binaries
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A second list of wide visual binaries
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Three-color surface photometry of a selected sample of early-type galaxies. I - Observations and data reduction
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UBV Photoelectric Photometry Catalogue (1986). III Errors and Problems on DM and HD Stars
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Transformation equations and other aids for VRI photometry
Transformations among VRI systems are commonly beset by Paschen-jumpeffects, for which fully satisfactory allowance has not previously beenmade. This paper describes two new techniques which are based on thework of Gutierrez-Moreno, and which allow fully for the effects of thePaschen jump. Values of E(V-R)/E(B-V) and E(R-I)/E(B-V) are also givenfor the Cousins system for a wide range of temperatures. These and thenew techniques contribute to a set of new transformation relations whichapply for most VRI systems; the status of the remaining systems isreviewed, and future work needed for them is described. Two majorsources of Cousins VRI data underlie the new relations; the consistencyof these sources is reviewed and found to be generally satisfactory,although more work on this question is needed. Finally, three tables oftransformed standard-star and other data are given for the Cousins andJohnson systems, and a description of ways to reproduce the latter ispresented.

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Standardization of Broadband Photometry of Equatorial Standards
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A UBVRI equatorial extinction star network
An equatorial-extinction star network, based on 1503 observations of 37stars, is presented. These results together with those of Crawford etal. (1971) provide a well-determined UBVRI extinction network.Identification charts are included.

Distances to eclipsing binaries. III - Masses, radii, and absolute magnitudes of 96 stars
Distances to, and absolute magnitudes of, 96 components of eclipsingbinaries with well-determined absolute dimensions have been computedusing V-R photometry. The calculations take into account interstellarreddening, which is estimated from existing UBV and uvby-betaphotometry, as well as photometric proximity effects. The resultingabsolute magnitudes, dimensions, and masses are compared with zero-agemain sequences predicted by theory. Theory is in good agreement with theobserved data for stars more massive than the sun if a composition (X,Y, Z) = (0.66 + or - 0.03, 0.303 + or - 0.03, 0.037 + or - 0.005) ischosen. The corresponding helium-to-hydrogen number ratio is 0.115 + or- 0.02, in agreement with previous estimates.

A UBV equatorial-extinction star network
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1971PASP...83..652C&db_key=AST

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Observation and Astrometry data

Constellation:Wasserschlange
Right ascension:08h48m18.30s
Declination:+00°33'18.1"
Apparent magnitude:7.24
Distance:216.92 parsecs
Proper motion RA:-4.6
Proper motion Dec:-11
B-T magnitude:9.204
V-T magnitude:7.403

Catalogs and designations:
Proper Names   (Edit)
HD 1989HD 75138
TYCHO-2 2000TYC 212-1202-1
USNO-A2.0USNO-A2 0900-06159361
HIPHIP 43224

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