J/ApJ/540/1016   K-band & NICMOS photometry of Trapezium Cluster (Luhman+, 2000)

The initial mass function of low-mass stars and brown dwarfs in young clusters. Luhman K.L., Rieke G.H., Young E.T., Cotera A.S., Chen H., Rieke M.J., Schneider G., Thompson R.I. <Astrophys. J. 540, 1016 (2000)> =2000ApJ...540.1016L 2000ApJ...540.1016L
ADC_Keywords: Clusters, open ; Stars, pre-main sequence ; Infrared sources ; Magnitudes ; Spectra, infrared Mission_Name: HST Keywords: infrared: stars - stars: evolution - stars: formation - stars: low-mass, brown dwarfs - stars: luminosity function, mass function - stars: pre-main-sequence Abstract: We have obtained images of the Trapezium Cluster (140"x140"; 0.3pc x 0.3pc) with the Hubble Space Telescope Near-Infrared Camera and Multi-Object Spectrometer (NICMOS). Combining these data with new ground-based K-band spectra (R=800) and existing spectral types and photometry, we have constructed an H-R diagram and used it and other arguments to infer masses and ages. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 189 320 Data for the Trapezium Cluster -------------------------------------------------------------------------------- See also: I/134 : Trapezium Multiple Systems (Salukvadze, 1978) J/A+A/299/39 : Orion Trapezium area ROSAT PSPC obs. I. (Geier+, 1995) J/AN/321/81 : Orion Trapezium area ROSAT PSPC obs. II. (Lohmann+, 2000) J/AJ/117/1375 : Orion Trapezium cluster (Simon+, 1999) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- [LRY2000] Sequential number 4- 6 A3 --- n_[LRY2000] [ghijkl ] Individual notes (1) 8- 14 A7 --- TCC Designations of McCaughrean & Stauffer, 1994AJ....108.1382M 1994AJ....108.1382M 15- 18 I4 --- [H97b] ? Designations of Hillenbrand, 1997AJ....113.1733H 1997AJ....113.1733H 19 A1 --- m_[H97b] [ab] Multiplicity index on [H97b] 21- 22 I2 h RAh Right ascension (J2000) 24- 25 I2 min RAm Right ascension (J2000) 27- 32 F6.3 s RAs Right ascension (J2000) 34 A1 --- DE- Declination sign (J2000) 35- 36 I2 deg DEd Declination (J2000) 38- 39 I2 arcmin DEm Declination (J2000) 41- 45 F5.2 arcsec DEs Declination (J2000) 47- 95 A49 --- SpTypel Previous spectral type determinations (2) 97-123 A27 --- IRType IR type (3) 125-133 A9 --- SpType Adopted spectral type 135-139 I5 K Teff ? Effective temperature 141-144 F4.2 mag AH ? Absorption in H band 146-155 F10.3 solLum Lbol ? Bolometric luminosity 157 A1 --- l_V-I Limit flag on V-I 158-162 F5.2 mag V-I ? V-I colour index (2) 164-168 F5.2 mag Imag ? I magnitude (2) 170 A1 --- l_m100-m160 Limit flag on 100-160 171-175 F5.2 --- m100-m160 ? F100W(0.8-1.4um)-F160W(1.4-1.8um) colour index (4) 177-181 F5.2 mag m160mag ? F160W (1.4-1.8um) magnitude 183-187 F5.2 mag Kmag ? K magnitude from McCaughrean & Stauffer, 1994AJ....108.1382M 1994AJ....108.1382M -------------------------------------------------------------------------------- Note (1): Individual notes: g: Member of a binary system that is resolved in the optical measurements while unresolved in the IR photometry. h: The spectral type assigned to source 97 applies to the composite system of 97, 100, and 101. i: Within a diffraction spike. j: Hillenbrand, 1997AJ....113.1733H 1997AJ....113.1733H k: Optical measurement listed for TCC046 probably includes both TCC039 and TCC046. l: Optical measurement listed for TCC073 includes both TCC070 and TCC073. Note (2): References for spectral types: T: Trumpler, 1931PASP...43..255T 1931PASP...43..255T Par: Parenago, 1954, Cat. II/171 J: Johnson, 1965ApJ...142..964J 1965ApJ...142..964J S: Strand, 1958ApJ...128...14S 1958ApJ...128...14S LA: Levato & Abt, 1976PASP...88..712L 1976PASP...88..712L or Abt & Levato, 1977PASP...89..797A 1977PASP...89..797A CK: Cohen & Kuhi, 1979ApJS...41..743C 1979ApJS...41..743C HT: Herbig & Terndrup, 1986ApJ...307..609H 1986ApJ...307..609H, and reference therein P: C. F. Prosser & J. R. Stauffer 1993, private communication vA: van Altena et al., 1988AJ.....95.1744V 1988AJ.....95.1744V Eetal: Edwards et al., 1993AJ....106..372E 1993AJ....106..372E Sam: Samuel 1993, Ph. D. thesis, Australian National Univ. Ham: Hamilton 1994, Masters thesis, Wesleyan University H: Hillenbrand, 1997AJ....113.1733H 1997AJ....113.1733H Hp: L. A. Hillenbrand 2000, private comm. (Hp). Note (3): The spectral type, K-band continuum veiling, and CO band head strength measured from the K-band spectra. The veiling at K is defined as r{K}=I2.2(IR excess)/I2.2(star), which is estimated from the spectra. The strength of the CO band head is given as a percentage increase in CO absorption over that of a dwarf of the same spectral type. Note (4): Blank entries indicate sources that are saturated or are too close to bright stars to be measured. The one exception is TCC003, which is not detected in the NICMOS data. -------------------------------------------------------------------------------- Table 2: Low-Mass Candidates in IC 348 -------------------------------------------------------------------------------- ID RA (J2000) DE R-I I J-H H-KS KS -------------------------------------------------------------------------------- 435 03 44 30.33 +32 11 33.9 1.45 18.95 1.20 0.85 14.24 603 03 44 33.43 +32 10 29.8 19.93 1.01 0.65 15.17 609 03 44 44.92 +32 09 34.7 21.20 0.99 0.36 16.89 618 03 44 43.92 +32 08 34.3 21.47 0.94 0.47 16.89 624 03 44 26.30 +32 08 08.7 21.83 1.01 0.67 16.43 -------------------------------------------------------------------------------- Note: The optical and IR photometry is from the work of Luhman 1999, Cat. J/ApJ/525/466 and Luhman et al. 1998ApJ...499..799L 1998ApJ...499..799L, respectively. -------------------------------------------------------------------------------- History: * 27-Nov-2000: From ApJ electronic version * 05-Mar-2001: the designation "TCC" corrected for 2 entries of table1 (dot removed in TCC names for entries 98 and 99)
(End) James Marcout, Patricia Bauer [CDS] 27-Nov-2000
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line