BD+36 2766 , the SIMBAD biblio

BD+36 2766 , the SIMBAD biblio (13 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.18CEST11:33:34


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Title First 3 Authors
1954AJ.....59..422B 36 34 Globular clusters. II. The tentative identification of the main sequence of population II from photoelectric observations in M 13. BAUM W.A.
1955ApJ...122..171A 34 93 The globular cluster M 13. ARP H.C. and JOHNSON H.L.
1956AJ.....61..254S 58 42 A photographic color-magnitude array of the globular cluster M13. SAVEDOFF M.P.
1966IzPul.181...93K viz 231 5 An investifation of globular cluster M 13. KADLA Z.I.
1969AJ.....74.1000M 4 6 172 The reddening of M 3, M 13, M 31, M 33 from photometry of late-type field stars. McCLURE R.D. and RACINE R.
1970ApJ...162..841S 1 108 720 Main-sequence photometry, color-magnitude diagrams, and ages for the globular clusters M 3, M 13, M 15 and M 92. SANDAGE A.
1979AJ.....84..774C 442 87 Astrometry in the globular cluster M 13. I. New proper motions and membership probabilities. CUDWORTH K.M. and MONET D.G.
1986PASP...98..102F 20 9 A photoelectric BVRI sequence in the field of the globular cluster NGC 6205 (M 13). FORBES D. and DAWSON P.C.
1997PASP..109.1193S 150 12 The Mount Wilson halo mapping project 1975-1985. I. The UBV(RI)$MW$ photometric system compared with other standard systems: the adopted trigonometric HR diagram in (R-I)$MW$ and (V-I)$MW$. SANDAGE A.
1997KFNT...13e..70R viz 49739 3 GPM - compiled catalogue of absolute proper motions of stars in selected areas of sky with galaxies. RYBKA S.P. and YATSENKO A.I.
2000AJ....119.2902O 103 6 Variable stars in M13. I. Positions and UBVRI photometry for variables, suspected variables, and comparison stars. OSBORN W.
2004A&A...418..357K viz 15       D               1 57786 7 The Pul-3 catalogue of 58483 stars in the Tycho-2 system. KHRUTSKAYA E.V., KHOVRITCHEV M.Y. and BRONNIKOVA N.M.
2019MNRAS.490.3158C viz 17       D               1 465834 28 A catalogue of stellar diameters and fluxes for mid-infrared interferometry. CRUZALEBES P., PETROV R.G., ROBBE-DUBOIS S., et al.

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