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SDSS J073728.47+472432.8 , the SIMBAD biblio (11 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST04:53:42 |
Bibcode/DOI | Score |
in Title|Abstract| Keywords |
in a table | in teXt, Caption, ... | Nb occurence | Nb objects in ref |
Citations (from ADS) |
Title | First 3 Authors |
---|---|---|---|---|---|---|---|---|---|
2011MNRAS.415.1188P | 15 | D | 1 | 122 | 32 | Study of galaxies in the Lynx-Cancer void. I. Sample description. | PUSTILNIK S.A. and TEPLIAKOVA A.L. | ||
2011MNRAS.417.1335P | 1382 | A | D | S X C F | 34 | 28 | 36 | Study of galaxies in the Lynx–Cancer void – III. New extreme low surface brightness dwarf galaxies. | PUSTILNIK S.A., MARTIN J.-M., TEPLIAKOVA A.L., et al. |
2013AJ....145..101K | 16 | D | 1 | 873 | 387 | Updated nearby galaxy catalog. | KARACHENTSEV I.D., MAKAROV D.I. and KAISINA E.I. | ||
2013AJ....146...46K | 16 | D | 1 | 824 | 78 | Star formation properties in the Local Volume galaxies via Hα and far-ultraviolet fluxes. | KARACHENTSEV I.D. and KAISINA E.I. | ||
2014AstBu..69..390K | O | 29 | 2 | New H alpha flux measurements in nearby dwarf galaxies. | KARACHENTSEV I.D. and KAISIN S.S. | ||||
2016MNRAS.463..670P | 16 | D | 1 | 86 | 7 | Study of galaxies in the Lynx-Cancer void - VII. New oxygen abundances. | PUSTILNIK S.A., PEREPELITSYNA Y.A. and KNIAZEV A.Y. | ||
2016A&A...596A..86P | 16 | D | 1 | 114 | 4 | Study of galaxies in the Lynx-Cancer void. VI. H I-observations with Nancay Radio Telescope. | PUSTILNIK S.A. and MARTIN J.-M. | ||
2018MNRAS.479..228K | 222 | D | X F | 5 | 18 | 9 | Angular momentum of dwarf galaxies. | KURAPATI S., CHENGALUR J.N., PUSTILNIK S., et al. | |
2021MNRAS.506.1346K | 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. | ||
2021MNRAS.507.3246H | 17 | D | 1 | 4479 | 15 | The nucleation fraction of local volume galaxies. | HOYER N., NEUMAYER N., GEORGIEV I.Y., et al. | ||
2024A&A...681A...8S | 20 | D | 1 | 61 | ~ | Effect of low-mass galaxy interactions on their star formation. | SUBRAMANIAN S., MONDAL C. and KALARI V. |