HD 283751 , the SIMBAD biblio

HD 283751 , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST08:17:35


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Title First 3 Authors
1961VeSon...5...87G 142 1 Photographische Untersuchungen an RW Aurigae-Sternen in den Dunkelgebieten von Taurus und Orion. GOETZ W.
1979AJ.....84.1872J 319 270 Proper motions of T Tauri variables and other stars associated with the Taurus-Auriga dark clouds. JONES B.F. and HERBIG G.H.
1980SvAL....6..397S 77 7 U, B, V, R, I stellar photometry in the field of the Taurus dark clouds. SLUTSKII V.E., STAL'BOVSKII O.I. and SHEVCHENKO V.S.
1984ApJ...282..508M 250 151 Magnetic field structure in the Taurus dark cloud. MONETI A., PIPHER J.L. and HELFER H.L.
1995A&AS..110..367N viz 82274 137 The Henry Draper Extension Charts: A catalogue of accurate positions, proper motions, magnitudes and spectral types of 86933 stars. NESTEROV V.V., KUZMIN A.V., ASHIMBAEVA N.T., et al.
2005A&A...438..769D viz 1380 87 Pre-main sequence star Proper Motion Catalogue. DUCOURANT C., TEIXEIRA R., PERIE J.-P., et al.
2010ApJS..186..259R viz 282       D     X         8 507 236 The Taurus Spitzer survey: new candidate Taurus members selected using sensitive mid-infrared photometry. REBULL L.M., PADGETT D.L., McCABE C.-E., et al.
2012ApJ...750..157C 15       D               2 65 60 The nature of transition circumstellar disks. III. Perseus, Taurus, and Auriga. CIEZA L.A., SCHREIBER M.R., ROMERO G.A., et al.
2013ApJ...771..110M viz 289       D     X C       7 363 17 B- and A-type stars in the Taurus-Auriga star-forming region. MOOLEY K., HILLENBRAND L., REBULL L., et al.
2015ApJS..219...20L viz 95       D       C       2 95 23 Outflows and bubbles in Taurus: star-formation feedback sufficient to maintain turbulence. LI H., LI D., QIAN L., et al.
1954ArA.....1..425A 13       D               1 1142 ~ A spectrophotometric investigation into bright and dark regions in Taurus. Part II. The catalogue. ADOLFSSON T.
2022ApJS..260...35W viz 18       D               1 452 5 Identification of New Classical Be Stars from the LAMOST Medium Resolution Survey. WANG L., LI J., WU Y., et al.

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