LP 415-1166 , the SIMBAD biblio

LP 415-1166 , the SIMBAD biblio (13 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.23CEST22:46:18


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Title First 3 Authors
1976AJ.....81..958V 320 265 Magnetic field structure in the vicinity of five dark cloud complexes. VRBA F.J., STROM S.E. and STROM K.M.
1979AJ.....84..548C 2 13 147 Two large-proper-motion Herbig-Haro objects. CUDWORTH K.M. and HERBIG G.
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.
1996ApJ...464..286C 74 56 X-ray-emitting T Tauri stars in the L1551 cloud. CARKNER L., FEIGELSON E.D., KOYAMA K., et al.
2001ApJS..133....1U viz 1480 79 The ASCA medium sensitivity survey (the GIS catalog project): source catalog. UEDA Y., ISHISAKI Y., TAKAHASHI T., et al.
2003A&A...403..187F 84 35 An XMM-Newton-based X-ray survey of pre-main sequence stellar emission in the L1551 star-forming complex. FAVATA F., GIARDINO G., MICELA G., et al.
2003ApJ...584..843B 94 95 X-rays from the vicinity of the protostar L1551 IRS 5: reflection or fast shocks. BALLY J., FEIGELSON E. and REIPURTH B.
2004A&A...420..945G viz         O           107 7 ISOCAM observations of the L1551 star formation region. GALFALK M., OLOFSSON G., KAAS A.A., et al.
2007A&A...468..353G viz 2328 298 The XMM-Newton extended survey of the Taurus Molecular Cloud (XEST). GUEDEL M., BRIGGS K.R., ARZNER K., et al.
2007A&A...468..477A 28 11 Statistics of superimposed flares in the Taurus molecular cloud. ARZNER K., GUEDEL M., BRIGGS K., et al.
2011A&A...527A.126P viz 15       D               11 16772 65 Cross-correlation of the 2XMMi catalogue with Data Release 7 of the Sloan Digital Sky Survey. PINEAU F.-X., MOTCH C., CARRERA F., et al.
2012ApJ...756...27L viz 15       D               1 4348 64 Classification of X-ray sources in the XMM-Newton serendipitous source catalog. LIN D., WEBB N.A. and BARRET D.
1995yCat.1098....0L viz 14       D               1 52092 ~ New Luyten Catalogue of stars with proper motions larger than two tenths of an arcsecond (NLTT). LUYTEN W.J.

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