scholarly journals R Coronae Borealis stars in the Galactic bulge discovered by EROS-2

2008 ◽  
Vol 481 (3) ◽  
pp. 673-690 ◽  
Author(s):  
P. Tisserand ◽  
J. B. Marquette ◽  
P. R. Wood ◽  
É. Lesquoy ◽  
J. P. Beaulieu ◽  
...  
2011 ◽  
Vol 529 ◽  
pp. A118 ◽  
Author(s):  
P. Tisserand ◽  
L. Wyrzykowski ◽  
P. R. Wood ◽  
A. Udalski ◽  
M. K. Szymański ◽  
...  

2005 ◽  
Vol 130 (5) ◽  
pp. 2293-2302 ◽  
Author(s):  
A. Zaniewski ◽  
Geoffrey C. Clayton ◽  
D. L. Welch ◽  
Karl D. Gordon ◽  
D. Minniti ◽  
...  

2000 ◽  
Vol 120 (2) ◽  
pp. 833-844 ◽  
Author(s):  
Solange V. Ramírez ◽  
Andrew W. Stephens ◽  
Jay A. Frogel ◽  
D. L. DePoy

1999 ◽  
Vol 117 (5) ◽  
pp. 2296-2307 ◽  
Author(s):  
Jay A. Frogel ◽  
Glenn P. Tiede ◽  
Leslie E. Kuchinski
Keyword(s):  

1998 ◽  
Vol 11 (1) ◽  
pp. 379-379
Author(s):  
P.L. Cottrell ◽  
L. Skuljan ◽  
P.M. Kilmartin ◽  
C. Gilmore ◽  
W.A. Lawson

For more than a decade we have been able to acquire and analyse a significant amount of photometric data of the highly variable R Coronae Borealis (RCB) stars. This has made been possible by a photometric service observing programme instigated at the Observatory. These photometric data have been combined with less extensive spectroscopic coverage, particularly of the decline phase of these stars. These have been supplemented by observations obtained at Mount Stromlo and Siding Spring Observatories for a radial velocity study. Significantly more spectroscopic observations are now being acquired with the development of a new medium resolution spectrograph at Mount John University Observatory. In this poster we will present recent photometric and spectroscopic results for a number of the RCB stars in our sample. This observational and analysis work can be used to provide further insight into the nature of these stars, their likely progeny and progenitors and the processes that are involved in the formation and evolution of the obscuring dust clouds which cause the decline phase.


2021 ◽  
Vol 2021 (07) ◽  
pp. E01
Author(s):  
Harrison Ploeg ◽  
Chris Gordon ◽  
Roland Crocker ◽  
Oscar Macias

1998 ◽  
Vol 11 (1) ◽  
pp. 560-561
Author(s):  
M. Grenon

As a preparation to the HIPPARCOS mission, a large observing programme on NLTT stars (propermotion > 0.18 ″/yr) was started in Genevaphotometry. The original programme consists of 10047 stars brighter than mR = 11.5, or mR = 12.5 if of colour class m. Among them, 7813 targets could be included in the HIPPARCOS programme, selected according to their observability and internal priorities in favour of large parallaxe stars (photometric distances < 100 pc) and high-velocity stars. The bulk of new nearby, halo, mild-metal poor and SMR stars in the HIP Catalogue originates from this proposal (N° 139). No less than 208 new nearby stars with π ≥ 40 mas were discovered south of δ +10°, the closest has π(HIP)= 182 mas. Radial velocities were obtained with CORAVEL at OHP and ESO. Most aspects of the early evolution of the Galaxy may be addressed with this sample. Here we discuss, as examples, the ages of the thick disk and of the galactic bulge.


2000 ◽  
Vol 536 (2) ◽  
pp. 798-815 ◽  
Author(s):  
C. Alcock ◽  
R. A. Allsman ◽  
D. R. Alves ◽  
T. S. Axelrod ◽  
A. C. Becker ◽  
...  

2010 ◽  
Vol 517 ◽  
pp. A44 ◽  
Author(s):  
S. Uttenthaler ◽  
M. Stute ◽  
R. Sahai ◽  
J. A. D. L. Blommaert ◽  
M. Schultheis ◽  
...  

Nature ◽  
1983 ◽  
Vol 301 (5897) ◽  
pp. 222-223 ◽  
Author(s):  
A. C. Fabian ◽  
J. E. Pringle ◽  
F. Verbunt ◽  
R. A. Wade

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