[MGA2005] H92alp 4 , the SIMBAD biblio

[MGA2005] H92alp 4 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST12:36:08


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Title First 3 Authors
2005A&A...432....1M 28 11 Multi-density model of the ionised gas in NGC 253 using radio recombination lines. MOHAN N.R., GOSS W.M. and ANANTHARAMAIAH K.R.
2017ApJ...849...81A 22 13 Diverse nuclear star-forming activities in the heart of NGC 253 resolved with 10-pc-scale ALMA images. ANDO R., NAKANISHI K., KOHNO K., et al.
2018ApJ...867L...6B 16       D               1 8 3 Evidence for the first extragalactic hydrogen recombination line maser in NGC 253. BAEZ-RUBIO A., MARTIN-PINTADO J., RICO-VILLAS F., et al.
2018ApJ...869..126L 19       D               1 23 70 Forming super star clusters in the central starburst of NGC 253. LEROY A.K., BOLATTO A.D., OSTRIKER E.C., et al.
2019ApJ...871..170M 950       D     X C       23 35 5 Fire in the heart: a characterization of the high kinetic temperatures and heating sources in the nucleus of NGC 253. MANGUM J.G., GINSBURG A.G., HENKEL C., et al.
2020MNRAS.491.4573R 16       D               1 24 ~ Super Hot Cores in NGC 253: witnessing the formation and early evolution of super star clusters. RICO-VILLAS F., MARTIN-PINTADO J., GONZALEZ-ALFONSO E., et al.
2020ApJ...897..176K viz 263       D     X         7 19 13 The molecular interstellar medium in the super star clusters of the starburst NGC 253. KRIEGER N., BOLATTO A.D., LEROY A.K., et al.
2021ApJ...912....4L 17       D               1 22 14 Outflows from super star clusters in the central starburst of NGC 253. LEVY R.C., BOLATTO A.D., LEROY A.K., et al.
2021ApJ...919..105M 17       D               3 28 6 Clustered star formation in the center of NGC 253 contributes to driving the ionized nuclear wind. MILLS E.A.C., GORSKI M., EMIG K.L., et al.
2022MNRAS.516.1094R 1464       D     X C F     33 36 2 On the thermal structure of the proto-super star cluster 13 in NGC 253. RICO-VILLAS F., GONZALEZ-ALFONSO E., MARTIN-PINTADO J., et al.
2024MNRAS.534.2499N 18       D               1 61 ~ Using 26 Al to detect ongoing self-enrichment in young massive star clusters. NOWAK K., KRAUSE M.G.H., SIEGERT T., et al.

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