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J/A+A/299/453 OH/IR stars photometry (Lepine+, 1995)
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OH/IR stars: near-infrared photometry, and discussion of the Mira-OH/IR sequence
Lepine J.R.D., Ortiz R., Epchtein N.
<Astron. Astrophys. 299, 453 (1995)>
=1995A&A...299..453L (SIMBAD/NED Reference)
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ADC_Keywords: Stars, masers; Photometry, infrared
Keywords: stars: AGB, post-AGB ; evolution ; circumstellar matter -
infrared: stars
Abstract:
This paper presents JHKL'M photometry of a new sample of OH/IR stars.
These data are merged with similar observations collected in the
literature in order to constitute a data base of near-infrared photometry
for 400 OH/IR stars. After removing from this sample the objects that are
unlikely to be AGB stars, we obtain a sequence of average OH/IR stars
with increasing values of the colour index K-L'. A simple model of a star
surrounded by a circumstellar shell is constructed in order to derive
basic parameters such as luminosity, radius, stellar temperature, optical
depth of the dust shell and mass loss rate. These parameters are found
to vary smoothly along the sequence of OH/IR stars, and the K-L' colour is
shown to describe almost completely the basic physical parameters of an
OH/IR star. The metallicity affects the OH-peak separation, but does not
play an important role in the definition of the other properties.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table1 37 405 Near-infrared counterparts of OH/IR stars
table2 74 383 Catalog of near-infrared photometry of
OH/IR stars
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Byte-by-byte Description of file: table1
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Bytes Format Units Label Explanations
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3- 13 A11 --- IRAS IRAS name
15- 16 I2 --- Ref Reference (1)
18- 37 A20 --- OtherRef Other reference (1)
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Note (1): 00=this work; 01=Fouque et al. 1992;
02=Epchtein et al. 1990; 03=Guglielmo et al. 1993;
04=Epchtein & Nguyen-Quang-Rieu 1982;
05=Le Bertre 1987; 06=Le Bertre 1991; 07=Braz & Epchtein 1982;
08=Le Bertre et al. 1984; 09=Epchtein et al. 1980;
10=Epchtein & Lepine; 1981; 11=Le Bertre et al. 1984;
12=Epchtein et al. 1987; 13=Braz & Epchtein 1987;
14=Whitelock & Feast 1984; 15=Whitelock 1985; 16=Whitelock et al.1986;
17=Gaylard & Whitelock 1988; 18=Gaylard et al. 1989;
19=Whitelock et al. 1991; 20=Feast et al. 1983; 21=Glass 1988;
22=Glass 1986; 23=Glass 1978; 24=Persi et al. 1990;
25=Persi & Ferrari-Toniolo 1984; 26=Manchado et al. 1989;
27=Garcia-Lario et al. 1990; 28=Garcia-Lario et al. 1993;
29=van der Veen 1988; 30=Blommaert et al. 1993; 31=Blommaert 1992;
32=Willems & de Jong 1982; 33=Evans & Beckwith 1977;
34=Engels et al. 1981; 35=Schultz et al. 1976; 36=Werner et al. 1989;
37=Wilson et al. 1972; 38=Jones et al. 1982; 39=Jones et al. 1983;
40=Lawrence et al. 1990; 41=Fix & Mutel 1984; 42=Allen et al. 1977;
43=Gosnell et al. 1979; 44=Persson & Campbell 1988;
45=Nyman et al. 1993; 46=Le Bertre 1993
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Byte-by-byte Description of file: table2
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Bytes Format Units Label Explanations
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1- 10 A10 --- IRAS IRAS name
11 A1 --- m_IRAS Multiplicity index on IRAS
13- 18 F6.2 deg LON Longitude
20- 25 F6.2 deg LAT Latitude
27- 32 F6.1 km/s Vlow Lowest velocity
34- 39 F6.1 km/s Vhigh Highest velocity
41- 44 F4.1 kpc Dist Distance
46- 50 F5.2 mag Kmag K magnitude
53- 56 F4.2 mag J-H []? J-H colour
59- 62 F4.2 mag H-K []? H-K colour
64- 68 F5.2 mag K-L []? K-L colour
70- 74 F5.2 mag L-M []? L-M colour
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References:
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(End) Patricia Bauer [CDS] 21-Feb-1995