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Francesca Annibali Luca Zampieri The point-like X-ray source HLX-1, hosted in the S0 galaxy ESO 243-49, is the brightest known ultraluminous X-ray source and likely the strongest intermediate-mass ...
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Email: francesca.annibali@inaf.it; Personal info. Orcid: 0000-0003-3758-4516; Latest papers on ADS (based on ORCID, see here how to claim missing papers)
Contatti. Stanza: B-3W4. Telefono: +39 051 6357 331. Email: francesca.annibali@inaf.it. Informazioni personali. Orcid: 0000-0003-3758-4516. Paper più recenti su ADS. (based on ORCID, see here how to claim missing papers) Anatomy of a Low-Metallicity Starburst, JWST Proposal.
Feb 2, 2017 · Francesca Annibali is at the Istituto Nazionale Di Astrofisica (INAF) — Bologna Observatory, via Ranzani 1, I-40127 Bologna, Italy., Francesca Annibali Authors
- Francesca Annibali
- francesca.annibali@oabo.inaf.it
- 2017
Jan 17, 2022 · Chemical and stellar properties of star-forming dwarf galaxies. Francesca Annibali, Monica Tosi (INAF-OAS Bologna) Dwarf galaxies are the least massive, most abundant, and most widely distributed type of galaxies. Hence, they are key to testing theories of galaxy and Universe evolution. Dwarf galaxies sufficiently close to have their gas and ...
The science team consists of Alessandra Aloisi and Marco Sirianni of the European Space Agency and Space Telescope Science Institute; Francesca Annibali,Jennifer Mack, and Roeland van der Marel of the Space Telescope Science Institute; Abhijit Saha of the National Optical Astronomy Observatories; and Gisella Clementini, Rodrigo Contreras ...
Sep 14, 2022 · For nearby (<20 Mpc) star-forming galaxies, Francesca Annibali and Monica Tosi round up what we know about their stellar and chemical properties. These objects resemble the earliest formed ...
