Release 11.12 ("Hergest Ridge")
Release 11.12 ("Hergest Ridge")
| Selected bibliography |
|
| Reference n. 1 (gc555) | |
| Author | Sharina, M. E.; Donzelli, C. J.; Davoust, E.; Shimansky, V. V.; Charbonnel, C. |
| Title | Gemini spectroscopy of the outer disk star cluster BH176 |
| Abstract | BH176 is an old metal-rich star cluster. It is spatially and kinematically consistent with belonging to the Monoceros Ring. It is larger in size and more distant from the Galactic plane than typical open clusters, and it does not belong to ... |
| Journal | Astronomy & Astrophysics, Volume 570, id.A48, 15 pp. |
| Year of publication: | 2018 |
| Tags | BH 176 |
| Reference n. 2 (gc281) | |
| Author | Davoust, E.; Sharina, M. E.; Donzelli, C. J. |
| Title | The globular cluster BH 176 revisited |
| Abstract | First classified as an open cluster, BH 176 lies in a crowded field at low galactic latitude. Later studies have labeled it a transition-type object, a metal-rich globular, or an open cluster, with distance estimates in the range of 15 to 8... |
| Journal | Astronomy & Astrophysics, Volume 528 |
| Year of publication: | 2011 |
| Tags | BH 176 |
| Reference n. 3 (gc233) | |
| Author | Bonatto, C.; Bica, E. |
| Title | Structural parameters of 11 faint Galactic globular clusters derived with 2MASS |
| Abstract | Structural parameters and the total MV magnitude are important properties for the characterisation of individual globular clusters. With the growth in statistics, especially of the intrinsically faint objects, the collective properties of t... |
| Journal | Astronomy and Astrophysics, Vol. 479, pp.741-750 |
| CM diagram | |
| Year of publication: | 2008 |
| Tags | IC 1257, Lynga 7, Terzan 4, Terzan 10, BH 176, 1636-283, ESO280-SC06, 2MASS-GC01, 2MASS-GC02, GLIMPSE-C01, AL 3 |
| Reference n. 4 (gc110) | |
| Author | Ortolani, S.; Bica, E.; Barbuy, B. |
| Title | BH 176 and AM-2: globular or open clusters? |
| Abstract | We have obtained VI photometry for two low Galactic latitude star clusters: BH 176 and AM-2, using the 2.2m and the 3.5m NTT telescopes at ESO. Their VI colour-magnitude diagrams reveal that: BH 176 may be a globular cluster, or a borderlin... |
| Journal | Astronomy and Astrophysics, 1995, v.300, p.726 |
| CM diagram |  |
| Year of publication: | 1995 |
| Tags | BH 176, cmd |
Query processed at 20:37, 29th April
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