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[SSA2010] 1446 , the SIMBAD biblio (12 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST09:55:45 |
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 |
---|---|---|---|---|---|---|---|---|---|
1982ApJS...49..405C | 266 | 84 | The cluster system of M 33. | CHRISTIAN C.A. and SCHOMMER R.A. | |||||
1992ApL....28..281I | 185 | ~ | Nonstellar objects in M 33. | IVANOV G.R. | |||||
1998AcA....48..455M | 157 | 47 | Identification and photometry of globular clusters in M31 and M33 galaxies. | MOCHEJSKA B.J., KALUZNY J., KROCKENBERGER M., et al. | |||||
2002AcA....52..453M | 61 | 13 | Spectral energy and age distributions for 51 globular cluster candidates. | MA J., ZHOU X., CHEN J., et al. | |||||
2007AJ....134..447S | 15 | D | 454 | 33 | A catalog of star cluster candidates in M 33. | SARAJEDINI A. and MANCONE C.L. | |||
2009ApJ...699..839S | 15 | D | 1 | 164 | 20 | Newly identified star clusters in M33. II. Radial Hubble space Telescope/Advanced camera for surveys fields. | SAN ROMAN I., SARAJEDINI A., GARNETT D.R., et al. | ||
2010ApJ...720.1674S | 15 | D | 2 | 2988 | 24 | Photometric properties of the M33 star cluster system. | SAN ROMAN I., SARAJEDINI A. and APARICIO A. | ||
2012AJ....144...41M | 15 | D | 1 | 394 | 11 | An updated catalog of M33 clusters and candidates: UBVRI photometry and some statistical results. | MA J. | ||
2012MNRAS.426.2427S | 15 | D | 1 | 169 | 8 | Newly identified star clusters in M33 - III. Structural parameters. | SAN ROMAN I., SARAJEDINI A., HOLTZMAN J.A., et al. | ||
2013AJ....145...88M | 16 | D | 1 | 460 | 6 | New UBVRI photometry of 234 M33 star clusters. | MA J. | ||
2015MNRAS.451.3400B | 16 | D | 1 | 91 | 15 | Evidence for temporal evolution in the M33 disc as traced by its star clusters. | BEASLEY M.A., SAN ROMAN I., GALLART C., et al. | ||
2022ApJ...933..156M | 18 | D | 1 | 64 | 3 | Dust Emission as a Function of Stellar Population Age in the Nearby Galaxy M33. | MALLORY K., CALZETTI D. and LIN Z. |