2005IAUC.8567....2O

Query : 2005IAUC.8567....2O

2005IAUC.8567....2O - IAU Circ., 8567, 2 (2005/July-0)

OTERO S. and HOWELL S.

Abstract (from CDS):

S. Otero, Buenos Aires, Argentina, reports that AS 325, an eclipsing binary (period 513 days), has entered a rapid decline phase and is currently near mid-eclipse; the current eclipse started on June 5, and eclipses last about 86 days. AS 325 is presently at V = 12.0, or 2 mag fainter then prior to eclipse, and over 1 mag fainter than during previous eclipses (IBVS 5608; http://www.astrouw.edu.pl/cgi-asas/asas_lc/185004-2624.3). S. Howell, WIYN Observatory, reports that spectra obtained during June 28-July 2 reveal that the H emission is weaker by 50 percent, while the Fe II emission remains constant, and the previously strong Ca II H and K absorption is nearly absent (Cool et al. 2005, PASP 117, 462). Spectra from July 1 show a slightly increasing blue continuum mainly consisting of emission lines and obvious TiO absorption in the red. Mid-eclipse is expected for July 18, and multicolor observations and additional spectra are needed to confirm that the cool component is the one that is being eclipsed. The Tycho Reference Catalogue (via SIMBAD) lists the position of AS 325 as R.A. = 18h50m03s.57, Decl. = -26o24'15".4 (equinox 2000.0).

Abstract Copyright: ∼

Journal keyword(s):

Simbad objects: 1

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Number of rows : 1

N	Identifier	Otype	ICRS (J2000) RA	ICRS (J2000) DEC	Mag U	Mag B	Mag V	Mag R	Mag I	Sp type	#ref 1850 - 2026	#notes
1	CD-26 13521	Be*	18 50 03.5694141888	-26 24 15.382929060		10.75	10.08			Bep	25	0

Query : 2005IAUC.8567....2O

Basic data :

CD-26 13521 -- Be Star

EB* (), * (CD,CPD,...), Em* (EM*,Hen,...), V* (NSV,V*), Be* (2003A&A), NIR (2MASS)

18 50 03.5694141888 -26 24 15.382929060 (Optical) [ 0.0182 0.0162 90 ] A 2020yCat.1350....0G

18 46 57.3214582123 -26 27 45.462984807 [ 0.0182 0.0162 90 ]

008.9606936334230 -11.4190068433123 [ 0.0182 0.0162 90 ]

-3.264 -9.607 [0.021 0.018 90] A 2020yCat.1350....0G

0.1873 [0.0214] A 2020yCat.1350....0G

Bep E 2003A&A...397..927P

B 10.75 [0.06] D 2000A&A...355L..27H

V 10.08 [0.04] D 2000A&A...355L..27H

G 9.676476 [0.007470] C 2020yCat.1350....0G

J 8.168 [0.029] C 2003yCat.2246....0C

H 7.520 [0.027] C 2003yCat.2246....0C

K 7.204 [0.021] C 2003yCat.2246....0C

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`CD-26 13521`	`2MASS J18500356-2624153`	`TIC 325751490`	`Gaia DR2 4072362542662424960`
`CPD-26 6567`	`NSV 24607`	`TYC 6867-437-1`	`Gaia DR3 4072362542662424960`
*`EM AS 325`**	`PPM 734474`	`UCAC2 21185695`	`Gaia DR1 4072362542662424960`
`GSC 06867-00437`	`SS73 175`	*`V V5569 Sgr`**
`Hen 3-1728`	*`SV BV 1732`**	`WRAY 15-1882`

References (25 between 1850 and 2026) (Total 25)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).

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`CD-26 13521`	`CPD-26 6567`	`GSC 06867-00437`	`2MASS J18500356-2624153`	`NSV 24607`
`PPM 734474`	`TYC 6867-437-1`	`UCAC2 21185695`	*`V V5569 Sgr`**	`Gaia DR2 4072362542662424960`
`Gaia DR3 4072362542662424960`	`Gaia DR1 4072362542662424960`

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