J/A+A/299/347 IRAS galaxies behind Taurus clouds (Chamaraux+, 1995)
A search for IRAS galaxies behind the Taurus molecular clouds.
CHAMARAUX P., KAZES I., SAITO M., YAMADA T., TAKATA T.
<Astron. Astrophys. 299, 347 (1995)>
=1995A&A...299..347C 1995A&A...299..347C (SIMBAD/NED Reference)
ADC_Keywords: Galaxies, IR; Radio sources; Redshifts
Keywords: surveys - galaxies: redshifts - infrared: galaxies -
large-scale structure of universe
Description:
We carried out a complete search for IRAS galaxies in the Taurus molecular
cloud region at l=169deg to 177deg and b=-19deg to -12deg. We selected a
total number of 36 galaxies and galaxy candidates and looked for the 21-cm
H I line in 25 objects; we detected H I emission in five of them including
one with previously unknown redshift. The spatial density of IRAS galaxies
with cz=4000 to 6000km/s is lower in this region than in the adjacent
regions at both sides along galactic longitude, where the Perseus
supercluster and the Gemini-Monoceros filament are respectively located.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table2 86 36 IRAS galaxies and galaxy candidates in the
Taurus molecular cloud region
table2.tex 74 102 TeX version of table2
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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- 15 A15 --- Name IRAS name
17- 23 F7.3 deg GLON Galactic longitude
25- 31 F7.3 deg GLAT Galactic latitude
33- 36 F4.2 Jy S12 Flux at 12 µm or density flux
37 A1 --- n_S12 [L] Note on S12
39- 42 F4.2 Jy S25 Flux at 25 µm or density flux
43 A1 --- n_S25 [L] Note on S25
45- 49 F5.2 Jy S60 Flux at 60 µm or density flux
51- 55 F5.2 Jy S100 Flux at 100 µm or density flux
56 A1 --- n_S100 [L] Note on S100
58- 67 A10 --- OptID Optical identification (1)
73- 76 I4 km/s cz []? Redshift velocity
77 A1 --- n_cz [*g] Note on redshift velocity (2)
81 A1 --- r_cz References for redshift velocity (3)
83- 86 A4 --- Detect Detection
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Note (1): The 15 objects indicated by s?, s/neb, gal/neb, and blank belong to
the objects with 'uncertain image' and FQ12=1 in Table 1.
IRAS 04112+2432, 04251+2132, and 04444+2353 are, respectively,
associated with CGCG 411.2+2432, UGC 3053, and UGC 3165 .
Note (2): g: galactic
*: we got the three unpublished redshift data denoted by * by private
communication; they are larger than 7000 km/s
Note (3): References:
a: Thonnard et al. 1978, AJ 83, 1564
b: Giovanelli & Haynes 1984, AJ 89, 758
c: Lu et al. 1990, ApJ 357, 388
d: Strauss et al. 1992, ApJS 83, 29
e: Strauss et al. 1994, private communication
f: Takata et al. 1994b, in preparation
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(End) Patricia Bauer [CDS] 08-Dec-1994