J/ApJS/99/551    BVI photometry of massive stars in M33 and M31 (Hunter+ 1995)

The massive star populations in ionized gas shells in M33 and M31 Hunter D.A., Boyd D.M., Hawley W.N. <Astrophys. J. Suppl. Ser. 99, 551 (1995)> =1995ApJS...99..551H 1995ApJS...99..551H
ADC_Keywords: Interstellar medium ; Photometry Keywords: galaxies: individual (M31, M33) - galaxies: ISM - galaxies: star clusters - galaxies: stellar content - stars: early-type Abstract: We present BVI photometry of the massive stars in and around five Halpha shells in M33 and two in M31. These data can be used to statistically compare the stellar population with ionization and formation requirements of the gas shell. We have counted the numbers of massive stars encircled by the shells and embedded within the gaseous structures and corrected these numbers statistically for background and foreground interlopers. We find that the stellar production exceeds the ionization requirements of the nebulae by factors of 4-10. Thus, it is reasonable that the shells are photoionized and that a large fraction of the ionizing photons escape into the rest of the galaxy. We have also compared the number of massive stars counted and extrapolated to 7M with the number required to form the shells according to a simple formation model. With one exception, we find that the number of stars estimated to be present exceeds the number required by the model for our assumptions of age and ambient gas density. This comparison and the morphology evident in Halpha images suggests that the modification of the interstellar medium by the massive stars in these regions has been far more complicated than is currently considered in formation models. There is evidence for multiple, and to some extent discreet, events in the production of the gas structures. A more detailed modeling will be necessary to adequately account for the stellar populations and Halpha morphology. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 71 2228 The photometry table3.dat 47 24 The groups and reddening -------------------------------------------------------------------------------- See also: J/ApJS/122/431 : Star Clusters in M33. I. (Chandar+, 1999) J/A+A/366/498 : HST VI photometry of M33 star clusters (Chandar+, 2001) J/AJ/121/861 : BVI photometry of central part of M33 (Macri+, 2001) J/AJ/121/870 : Variables in the central part of M33 BVI phot. (Macri+, 2001) J/AJ/110/1649 : HST VI photometry near the M33 nucleus (Mighell+ 1995) J/AJ/110/2715 : UBV photometry in NGC 6822, M31 and M33 (Massey+ 1995) J/ApJ/324/172 : M31 UBVR photometry (Hodge+, 1988) J/ApJS/118/177 : JHK photometry of M31 spiral arm (Kodaira+, 1998) J/ApJ/504/113 : F175W and F275W photometry of M31 and M32 (Brown+, 1998) Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Region The region in M33 or M31 10 I1 --- Group *Group identification number within region 11- 13 I3 --- Star Star identification number within the group 15- 21 F7.2 pix Xpos *X pixel coordinate 23- 29 F7.2 pix Ypos *Y pixel coordinate 31- 36 F6.2 mag Vmag V magnitude 38- 43 F6.2 mag e_Vmag Uncertainty in V 45- 50 F6.2 mag B-V *[]?=100.00 B-V color 52- 57 F6.2 mag e_B-V *[]?=100.00 Uncertainty in B-V color 59- 64 F6.2 mag V-I *[]?=100.00 V-I color 66- 71 F6.2 mag e_V-I *[]?=100.00 Uncertainty in V-I color -------------------------------------------------------------------------------- Note on Group: See Table 3 for descriptions of the groups. Note on Xpos, Ypos: The X,Y pixel coordinates are relative to the long V-band image shown in figure 1 (plates 11-16) of the printed paper. Note on B-V, e_B-V, V-I, e_V-I: A magnitude of 100.00 indicates that the star was not measured through that filter. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Region The region in M33 or M31 10 I1 --- Group Group identification number within region 13- 42 A30 --- Comment Comment on the group 44- 47 F4.2 --- E(B-V) []? Reddening -------------------------------------------------------------------------------- Origin: AAS CD-ROM series, Volume 5, 1995 Lee Brotzman [ADS] 31-Aug-95
(End) [CDS] 02-Feb-1996
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