Cl Alicante 10 , the SIMBAD biblio

Cl Alicante 10 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST14:36:18

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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
2012A&A...539A.100G 51 26 A third cluster of red supergiants in the vicinity of the massive cluster RSGC 3. GONZALEZ-FERNANDEZ C. and NEGUERUELA I.
2014A&A...564L...9R viz 39           X         1 29 15 Massive open star clusters using the VVV survey. III. A young massive cluster at the far edge of the Galactic bar. RAMIREZ ALEGRIA S., BORISSOVA J., CHENE A.N., et al.
2014A&A...567A..66R 39           X         1 54 3 Masgomas-4: Physical characterization of a double-core obscured cluster with a massive and very young stellar population. RAMIREZ ALEGRIA S., MARIN-FRANCH A. and HERRERO A.
2014A&A...571A..32M 40           X         1 17 39 The formation of the W43 complex: constraining its atomic-to-molecular transition and searching for colliding clouds. MOTTE F., NGUYEN LUONG Q., SCHNEIDER N., et al.
2019A&A...629A.117O 1462 T   A D     X C       35 19 ~ Stellar population astrophysics (SPA) with the TNG. GIANO-B spectroscopy of red supergiants in Alicante 7 and
Alicante 10. 		ORIGLIA L., DALESSANDRO E., SANNA N., et al.
2020MNRAS.495L.102E 16       D               1 18 ~ On ageing star clusters using red supergiants independent of the fraction of interacting binary stars. ELDRIDGE J.J., BEASOR E.R. and BRITAVSKIY N.
2020A&A...643A..12C viz 41           X         1 25 ~ Stellar Population Astrophysics (SPA) with TNG. The old open clusters Collinder 350, Gulliver 51, NGC 7044, and Ruprecht 171. CASALI G., MAGRINI L., FRASCA A., et al.
2023AJ....165..212A 392     A D     X         10 6 ~ To Be or Not to Be: Alicante-8, a Cluster or Not? ASA'D R., IVANOV V.D., NEGUERUELA I., et al.
2024AJ....167..230C 511       D     X   F     11 52 ~ Is the RSGC4 (Alicante 8) Cluster a Real Star Cluster? Peculiar Radial Velocities of Red Supergiant Stars. CHUN S.-H., MYEONG G., LEE J.-J., et al.

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