Astronomical Data Center
ADC/CDS Standard Document for Catalog:
/journal_tables/AJ/122/248/
The following is the "ReadMe" document that describes this ADC catalog. You can access the files described here in three ways:
J/AJ/122/248 h and chi Per UBVI,H{alpha} photometry (Keller+, 2001)
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UBVI and H{alpha} photometry of the h and {chi} Persei cluster.
Keller S.C., Grebel E.K., Miller G.J., Yoss K.M.
<Astron. J. 122, 248 (2001)>
=2001AJ....122..248K
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ADC_Keywords: Clusters, open ; Photometry, UBVRI ; Photometry, H-alpha ;
Stars, Be
Keywords: open clusters and associations: individual (NGC 869, NGC 884) -
stars: emission-line, Be - stars: evolution - techniques: photometric
Abstract:
UBVI and H{alpha} photometry is presented for 17319 stars in vicinity
of the young double cluster h and {chi} Persei. Our photometry extends
over a 37'x1{deg} field centered on the association. We construct
reddening contours within the imaged field. We find that the two
clusters share a common distance modulus of 11.75+/-0.05 and ages of
log[age(yr)]=7.1+/-0.1. From the V-H{alpha} color, a measure of the
H{alpha} emission strength, we conduct a survey for emission line
objects within the association. We detect a sample of 33 Be stars,
eight of which are new detections. We present a scenario of
evolutionary enhancement of the Be phenomenon to account for the peak
in Be fraction toward the top of the main sequence in the population
of h and {chi} Persei and similar young clusters.
UBVI and H{alpha} photometry was performed on five nights between 1999
August 17 and 25 at the San Diego State University Mount Laguna
Observatory with the 1m telescope and a Loral 2048x2048 CCD.
Objects:
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RA (2000) DE Designation(s)
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02 22 24 +57 07.0 NGC 884
02 19 00 +57 09.0 NGC 869
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File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table1.dat 100 5 Atmospheric extinction coefficients and photometric
zero points from the present study
table2.dat 74 17315 Photometric data
table4.dat 74 33 Be stars detected within the field of h and {chi} Per
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See also:
J/A+A/372/477 : ubvy{beta} photometry of h + chi Persei (Marco+, 2001)
J/A+AS/119/271 : Be stars uvby{beta} photometry (Fabregat+, 1996)
Byte-by-byte Description of file: table1.dat
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Bytes Format Units Label Explanations
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1- 10 A10 "YYYY/MM/DD" Date Observation date
12- 16 F5.3 mag k1,V Atmospheric extinction coefficient in V band
18- 22 F5.3 mag e_k1,V rms uncertainty on k1,V
24- 28 F5.3 mag k1,B Atmospheric extinction coefficient in B band
30- 34 F5.3 mag e_k1,B rms uncertainty on k1,B
36- 39 F4.2 mag k1,U Atmospheric extinction coefficient in U band
41- 44 F4.2 mag e_k1,U rms uncertainty on k1,U
46- 50 F5.3 mag K1,I Atmospheric extinction coefficient in I band
52- 56 F5.3 mag e_K1,I rms uncertainty on k1,I
58- 62 F5.3 mag ksiV Photometric zero point in V band
64- 68 F5.3 mag e_ksiV rms uncertainty on ksiV
70- 74 F5.3 mag ksiB Photometric zero point in B band
76- 80 F5.3 mag e_ksiB rms uncertainty on ksiB
82- 85 F4.2 mag ksiU Photometric zero point in U band
87- 90 F4.2 mag e_ksiU rms uncertainty on ksiU
92- 96 F5.3 mag ksiI Photometric zero point in I band
97-100 F4.2 mag e_ksiI rms uncertainty on ksiI
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Byte-by-byte Description of file: table2.dat table4.dat
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Bytes Format Units Label Explanations
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1- 5 I5 --- [KGM2001] Identification number
7- 15 F9.3 pix Xpix X pixel position (1)
17- 25 F9.3 pix Ypix Y pixel position (1)
28- 33 F6.3 mag Vmag The V-band magnitude
36- 41 F6.3 mag U-B The U-B color
44- 49 F6.3 mag B-V The B-V color
52- 57 F6.3 mag V-I The V-I color
60- 65 F6.3 mag V-Ha The V-H{alpha} color
67- 68 A2 --- Be [Be] Be: Be star
71- 74 I4 --- Oos ? The Oosterhoff (1937AnLei..17a...1O)
identification number (2)
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Note (1): The scale is 1 pix = 0.399"
Note (2): Identifications:
NGC 869 NNNN (for Nos 1-1640, 4000-4090), h Per
NGC 884 NNNN (for Nos 1641-2987, 7001-7125), chi Per
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History:
From electronic version of the journal
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(End) Greg Schwarz [AAS], Patricia Bauer [CDS] 14-Jan-2002
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