LEDA 2576103 , the SIMBAD biblio

LEDA 2576103 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST11:33:57


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Title First 3 Authors
2003A&A...412...45P viz 15       D               1 956189 750 HYPERLEDA. I. Identification and designation of galaxies. PATUREL G., PETIT C., PRUGNIEL P., et al.
2009A&A...496..191H viz 15       D               1 868 29 Spectral analysis of 636 white dwarf-M star binaries from the Sloan Digital Sky Survey. HELLER R., HOMEIER D., DREIZLER S., et al.
2010MNRAS.402..620R viz 15       D               1 1865 115 Post-common envelope binaries from SDSS - VII. A catalogue of white dwarf-main sequence binaries. REBASSA-MANSERGAS A., GANSICKE B.T., SCHREIBER M.R., et al.
2017A&A...602A.119M 16       D               1 57 37 The M 101 group complex: new dwarf galaxy candidates and spatial structure. MULLER O., SCALERA R., BINGGELI B., et al.
2018MNRAS.479.4136K viz 16       D               1 1019 3 Morphological properties of galaxies in different Local Volume environments. KARACHENTSEV I.D., KAISINA E.I. and MAKAROV D.I.
2019MNRAS.486.3697K 16       D               1 85 ~ 'Scraggy' dark haloes around bulge-less spiral. KARACHENTSEV I.D. and KARACHENTSEVA V.E.
2020AJ....159...37K 387       D     X C       9 36 ~ Neutral hydrogen observations of low surface brightness galaxies around M101 and NGC 5485. KARUNAKARAN A., SPEKKENS K., BENNET P., et al.
2020MNRAS.495.3592K viz 16       D               1 316 ~ Statistics and properties of emission-line regions in the local volume dwarf galaxies. KARACHENTSEV I.D. and KAISIN S.S.
2021MNRAS.506.1346K viz 17       D               1 482 ~ Local Volume late-type galaxies with an extreme ratio of H α-to-FUV SFRs. KARACHENTSEV I.D., KAISINA E.I. and KAISIN S.S.
2023A&A...678A..16K 17       D               4 75 ~ The M 101 galaxy group as a node in a nearby cosmic filament. KARACHENTSEVA V.E., KARACHENTSEV I.D., KAISINA E.I., et al.
2025MNRAS.537L..21K 19       D               1 63 ~ New radial velocities for 40 nearby dwarf galaxies. KARACHENTSEV I.D., CHAZOV M.I. and KAISIN S.S.

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