III/177 H-alpha emission stars in the Orion region (Wiramihardja+ 1993)
Survey Observations of Emission-line Stars in the Orion Region
I. The Kiso Area A-0904
Wiramihardja S.D., Kogure T., Yoshida S., Ogura K., Nakano M.
<Publ. Astron. Soc. Japan 41, 155 (1989)> (Part I)
=1989PASJ...41..155W 1989PASJ...41..155W
II. The Kiso Area A-0903
Kogure T., Yoshida S., Wiramihardja S.D., Nakano M., Iwata T., Ogura K.
<Publ. Astron. Soc. Japan 41, 1195 (1989)> (Part II)
=1989PASJ...41.1195K 1989PASJ...41.1195K
III. The Kiso Area A-0975 and A-0976
Wiramihardja S.D., Kogure T., Yoshida S., Nakano M., Ogura K., Iwata T.
<Publ. Astron. Soc. Japan 43, 27 (1991)> (Part III)
=1991PASJ...43...27W 1991PASJ...43...27W
IV. The Kiso Area A-1047 and A-1048
Wiramihardja S.D., Kogure T., Ogura K., Yoshida S., Nakano M.
<Publ. Astron. Soc. Japan 45, 643 (1993)> (Part IV)
=1993PASJ...45..643W 1993PASJ...45..643W
ADC_Keywords: Stars, emission
Abstract:
Extensive survey observations were carried out for H-alpha emission
stars in six Kiso Areas in the Orion region. The observations were
made using mainly the Kiso Schmidt telescope, and partly using the
CTIO Curtis Schmidt telescope. Our surveys extends the limiting
magnitude to V=17.5 over an area of 150 square degrees, and the total
number of detected H-alpha emission stars were 1157. The celestial
coordinates and the V magnitudes were measured along with an eye
estimation of the H-alpha intensities. The identification from the
previous observations were also made. The brightness distribution,
which is peaked around V=15, suggests that they are probable
candidates of T Tauri-type stars.
File Summary:
--------------------------------------------------------------------------------
FileName Lrecl Records Explanations
--------------------------------------------------------------------------------
ReadMe 80 . This file
catalog.dat 98 1214 H-alpha emission-line stars in Ori region
notes.dat 58 68 Notes to flagged stars
--------------------------------------------------------------------------------
Byte-by-byte Description of file: catalog.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 2 I2 --- area [03/76] Area number (1)
3- 5 I3 --- seq [1/415] Serial number in each area in
increasing R.A. order at epoch of 1950.0.
7- 8 I2 h RAh [5] right ascension (hours) (B1950)
10- 11 I2 min RAm right ascension (minutes)
13- 16 F4.1 s RAs right ascension (seconds)
18 A1 --- DE- [±]! declination sign
19- 20 I2 deg DEd [0/12] declination (degrees) (B1950)
22- 23 I2 arcmin DEm declination (minutes)
25- 26 I2 arcsec DEs declination (seconds)
28 I1 --- INT1 [0/9] Estimated H-alpha emission intensity (2)
30 I1 --- INT2 [0/9]? Second estimated H-alpha emission
intensity
32 I1 --- INT3 [0/9]? Third estimated H-alpha emission
intensity
34- 37 F4.1 mag Vmag [6.5/18.6]?=99.9 V magnitude (3)
39- 98 A60 --- Notes Identification with the previous surveys (4)
--------------------------------------------------------------------------------
Note (1): The 6 area numbers are as follows:
-----------------------------------------------
Kiso Area central position paper
R.A. Dec.
----------------------------------------------
03 A0903 5:20 0:00 II
04 A0904 5:40 0:00 I
75 A0975 5:20 - 5:00 III
76 A0976 5:40 - 5:00 III
47 A1047 5:20 -10:00 IV
48 A1048 5:40 -10:00 IV
-----------------------------------------------
Note (2): For A0904 and A0976, at three and two epochs of observations,
respectively. The scale of emission intensity is given by the six
grades of 5 (very strong), 4 (strong), 3 (medium), 2 (weak), 1 (very
weak), 0 (absent or doubtful), and 9 means that it lies out of area
on the CTIO plates.
Note (3): "99.9" indicates unreliable magnitude measurement by several
causes, such as unseparated double star image, saturated bright star
image, contamination by nebulosities.
"=>" indicates another number of the same
object appearing in this catalogue
beforehand; a "*" indicates a note in
file notes.dat (4)
Note (4): "=>" indicates another number of the same object appearing
in this catalogue beforehand
"*" indicates a note in file notes.dat
Abbreviations used for the headings in the respective current ID numbers
are given below:
--------------------------------------------------------------------------
B Bernes, =1977A&AS...29...65B 1977A&AS...29...65B
Brun Brun, =1935POLyo...1...12B 1935POLyo...1...12B
H Haro, =1953ApJ...117...73H 1953ApJ...117...73H
HM Haro & Moreno(1953) Bol.Obs.Tonantzintla Tacubaya 7,11.
=1953BOTT....1g..11H 1953BOTT....1g..11H
HBC Herbig & Bell (1988) Lick Obs. Bulletin No.111.
=1988LicOB1111....1H 1988LicOB1111....1H; Catalog V/73
HK Herbig & Kuhi =1963ApJ...137..398H 1963ApJ...137..398H
IRAS IRAS Point Source Catalog, Catalog II/125
L LkHa-number (Herbig & Kuhi =1963ApJ...137..398H 1963ApJ...137..398H;
Herbig & Rao 1972ApJ...174..401H 1972ApJ...174..401H).
M78/ Strom et al. =1975ApJ...196..489S 1975ApJ...196..489S
NK Nakajima et al. =1986MNRAS.221..483N 1986MNRAS.221..483N
NGC2068 Sellgren =1983AJ.....88..985S 1983AJ.....88..985S
OH Ogura & Hasegawa =1983PASJ...35..299O 1983PASJ...35..299O
P Parenago (1954) Trudy Sternberg Astr. Inst. 25,1.
=1954TrSht..25....1P 1954TrSht..25....1P ; Catalog II/171
PC Parsamyan & Chavira (1982) Bol.del Inst. de Tonantzintla 3,69.
San Sanduleak =1971PASP...83...95S 1971PASP...83...95S
SSV Strom et al. =1976AJ.....81..308S 1976AJ.....81..308S
St Stephenson =1986ApJ...300..779S 1986ApJ...300..779S
STR Strom et al. =1989ApJS...71..183S 1989ApJS...71..183S
Ton rapid variables found by Haro & Morgan =1953ApJ...118...16H 1953ApJ...118...16H;
Haro (1954) Bol Ton y Tac 2, nr 11, 11., and Haro & Rivera
Terrazas (1954) Bol Ton y Tac 1, nr 10, 3.
V Variable stars.
X Strom et al. =1990ApJ...362..168S 1990ApJ...362..168S
--------------------------------------------------------------------------
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Byte-by-byte Description of file: notes.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 2 I2 --- area Area number, as in catalog
3- 5 I3 --- seq Serial number, as in catalog
8- 58 A51 --- Text Text of note
--------------------------------------------------------------------------------
Historical Notes:
* 11-Aug-1994: The machine-readable version of this catalogue was compiled
by M. Nakano at Oita University, and reformatted and documented at the
Astronomical Data Analysis Center, the National Astronomical
Observatory of Japan.
* 24-Feb-1998: the notes have been gathered into the notes.dat file.
(F. Ochsenbein, CDS)
(End) S.Nishimura, K.Nakajima [ADAC/NAOJ] 11-Aug-1994