[vsnet-chat 7166] Re: Sequence for new MACHO R CrB star
Mati Morel
morel at ozemail.com.au
Fri Jul 29 10:04:38 JST 2005
Hi all,
A couple of these new RCB stars are about 14.3V at maximum, but as luck
would have it, one happens to lie within a CCD field imaged by Arne Henden,
USNOFS. In fact it lies only 20" from a recent nova, V5114 Sgr (2004). I have
extracted some useful comparison stars from Arne's .dat file.
MACHO*18:19:33.9-28:35:58 (name = 135.27132.51)
Position (2000) : 18:19:33.77 -28:35:58.0 from V5114SGR.dat
V = 14.404 (-0.006) B-V = 1.761 (-0.015)
Star # RA2000 DEC2000 V Verr B-V B-Verr
===============================================
1 18:19:35.94 -28:35:37.9 13.385 0.005 0.648 0.001
2 18 19 30.95 -28 36 29.3 13.641 0.048 1.753 0.025
3 18 19 33.68 -28 36 24.6 13.934 0.020 1.336 0.018
4 18 19 37.28 -28 36 28.0 14.242 0.042 1.689 0.019
5 18 19 34.47 -28 35 55.0 14.728 0.013 1.513 0.023
6 18 19 36.23 -28 35 25.1 14.908 0.003 1.829 0.002
7 18 19 34.48 -28 35 09.1 15.467 0.067 1.945 0.029
Notes: V5114 Sgr position , from .dat file,
18 19 32.19 -28 36 35.3
All of these stars lie in the small field chart, downloadable from
the URL below.
Regards,
Mati Morel
morel at ozemail.com.au
----- Original Message -----
Subject: [vsnet-chat 7161] New R CrB stars from MACHO survey
> New R CrB stars from MACHO survey
>
> Most of the objects are rather faint, but at least a few of them are
> within reach of moderate-size telescopes (especially with CCDs). Use the
> MACHO names (long!) when reporting observations.
>
> Paper: astro-ph/0507554
> Date: Fri, 22 Jul 2005 21:28:49 GMT (197kb)
>
> Title: Discovery of Five New R Coronae Borealis Stars in the MACHO Galactic
> Bulge Database
> Authors: A. Zaniewski, Geoffrey C. Clayton, D. L. Welch, Karl D. Gordon, D.
> Minniti, and K. H. Cook
> Comments: 16 pages, 5 figures, AJ in press High resolution versions of Figures
> 1 and 2 can be downloaded from
> http://morpheus.phys.lsu.edu/~gclayton/figs.pdf
> We have identified five new R Coronae Borealis (RCB) stars in the Galactic
> bulge using the MACHO Project photometry database, raising the total number of
> known Galactic RCB stars to about 40. We have obtained spectra to confirm the
> identifications. The fact that four out of the five newly identified RCB stars
> are ``cool'' (T(eff) < 6000 K) rather than ``warm'' (T(eff) > 6000 K) suggests
> that the preponderance of warm RCB stars among the existing sample is a
> selection bias............
> \\ ( http://arXiv.org/abs/astro-ph/0507554 , 197kb)
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