(Q59110354)

L. Morbidelli

30

0 references

Rodolfo Smiljanic

R. Smiljanic

6

0 references

Rosanna Sordo

R. Sordo

9

0 references

Loredana Prisinzano

L. Prisinzano

31

0 references

Laura Magrini

L. Magrini

5

0 references

Sofia Randich

S. Randich

20

0 references

Carmela Lardo

C. Lardo

36

0 references

Simone Zaggia

S. Zaggia

18

0 references

Antonella Vallenari

A. Vallenari

7

0 references

Ettore Flaccomio

E. Flaccomio

22

0 references

Elena Pancino

E. Pancino

25

0 references

Monica Tosi

M. Tosi

8

0 references

Douglas Geisler

13

D. Geisler

0 references

Sergey Koposov

23

S. E. Koposov

0 references

S. Blanco-Cuaresma

11

S. Blanco-Cuaresma

0 references

Tristan Cantat-Gaudin

2

T. Cantat Gaudin

0 references

Eileen Friel

4

E. Friel

0 references

G. Tautvaišienė

10

G. Tautvaišienė

0 references

author name string

P. Donati

1

0 references

A. Bragaglia

3

0 references

M. T. Costado

12

0 references

N. Mowlavi

15

0 references

C. Muñoz

16

0 references

I. San Roman

17

0 references

G. Gilmore

19

0 references

T. Bensby

21

0 references

A. J. Korn

24

0 references

A. Recio-Blanco

26

0 references

E. Franciosini

27

0 references

P. de Laverny

28

0 references

J. Lewis

29

0 references

G. Sacco

32

0 references

C. C. Worley

33

0 references

A. Hourihane

34

0 references

P. Jofré

35

0 references

E. Maiorca

Astronomy and Astrophysics

37

0 references

language of work or name

English

0 references

publication date

January 2014

0 references

published in

1 reference

SIMBAD

volume

561

1 reference

SIMBAD

page(s)

94–94

1 reference

NGC 2849 and NGC 6134: two more BOCCE open clusters★

SIMBAD

cites work

1 reference

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The effect of stellar rotation on colour-magnitude diagrams: on the apparent presence of multiple populations in intermediate age stellar clusters

21 January 2018

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The Bologna Open Cluster Chemical Evolution Project: Midterm Results from the Photometric Sample

21 January 2018

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The relationship between infrared, optical, and ultraviolet extinction

21 January 2018

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High-resolution spectroscopy of the old open cluster Collinder 261: abundances of iron and other elements

21 January 2018

1 reference

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Asteroseismology of the open clusters NGC 6791, NGC 6811, and NGC 6819 from 19 months of Kepler photometry

21 January 2018

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New catalogue of optically visible open clusters and candidates

21 January 2018

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The anticentre old open clusters Berkeley 27, Berkeley 34 and Berkeley 36: new additions to the BOCCE project★

21 January 2018

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The Old Open Clusters of the Milky Way

21 January 2018

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Evolutionary tracks and isochrones for low- and intermediate-mass stars: From 0.15 to 7 M?, and from Z=0.0004 to 0.03

21 January 2018

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Can rotation explain the multiple main-sequence turn-offs of Magellanic Cloud star clusters?

21 January 2018

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Age determination of six intermediate-age Small Magellanic Cloud star clusters with HST/ACS

21 January 2018

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Overlapping abundance gradients and azimuthal gradients related to the spiral structure of the Galaxy

21 January 2018

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The evolution of the Galactic metallicity gradient from high-resolution spectroscopy of open clusters

21 January 2018

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Asteroseismology of old open clusters with Kepler: direct estimate of the integrated red giant branch mass-loss in NGC 6791 and 6819

21 January 2018

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Chemical abundance analysis of the open clusters Cr 110, NGC 2099 (M 37), NGC 2420, NGC 7789, and M 67 (NGC 2682)

21 January 2018

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The effects of differential reddening and stellar rotation on the appearance of multiple populations in star clusters: the case of Trumpler 20

21 January 2018

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A synthetic view on structure and evolution of the Milky Way

21 January 2018

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Homogeneous photometry and star counts in the field of 9 Galactic star clusters

21 January 2018

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The Two Micron All Sky Survey (2MASS)

21 January 2018

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The old open clusters Berkeley 32 and King 11

21 January 2018

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The Victoria‐Regina Stellar Models: Evolutionary Tracks and Isochrones for a Wide Range in Mass and Metallicity that Allow for Empirically Constrained Amounts of Convective Core Overshooting

21 January 2018

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