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| Query : 2004MNRAS.347L..57G |
2004MNRAS.347L..57G - Mon. Not. R. Astron. Soc., 347, L57-L60 (2004/January-3)
LX-SFR relation in star-forming galaxies.
GILFANOV M., GRIMM H.-J. and SUNYAEV R.
Abstract (from CDS):
However, the most important conclusion from our comparison is that, after the data are corrected for the `LMXB contamination', the two data sets become consistent with each other, despite differences in their content, variability effects, adopted source distances, X-ray fluxes and SFR determinations, and also in the cosmological parameters used in interpreting the Hubble Deep Field North (HDF-N) data. They also agree well, both in the low- and high-SFR regimes, with the predicted LX-SFR dependence derived from the parameters of the `universal' high-mass X-ray binary (HMXB) luminosity function. This encouraging result emphasizes the potential of the X-ray luminosity as an independent SFR indicator for normal galaxies.
Abstract Copyright: 2004 RAS
Journal keyword(s): galaxies: starburst - X-rays: binaries - X-rays: galaxies
Simbad objects: 29
| Number of rows : 29 |
| N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2026 |
#notes |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | NGC 55 | rG | 00 14 53.602 | -39 11 47.86 | 8.54 | 8.58 | 7.87 | 7.84 | ~ | 828 | 2 | |
| 2 | NAME SMC | G | 00 52 38.0 | -72 48 01 | 2.79 | 2.2 | ~ | 12317 | 1 | |||
| 3 | M 74 | G | 01 36 41.7451236624 | +15 47 01.107512304 | 10.52 | 10.00 | 9.46 | 9.16 | ~ | 1934 | 1 | |
| 4 | NGC 891 | H2G | 02 22 32.907 | +42 20 53.95 | 11.08 | 10.81 | 9.93 | 7.86 | ~ | 1741 | 2 | |
| 5 | IC 342 | AGN | 03 46 48.514 | +68 05 45.98 | 10.5 | ~ | 1579 | 1 | ||||
| 6 | NGC 1569 | rG | 04 30 49.186 | +64 50 52.52 | 11.72 | 11.86 | 11.03 | ~ | 1297 | 3 | ||
| 7 | NGC 1672 | SyG | 04 45 42.552 | -59 14 50.68 | 10.29 | 10.53 | 9.68 | 9.53 | 10.2 | ~ | 461 | 2 |
| 8 | NGC 1808 | Sy2 | 05 07 42.343 | -37 30 46.98 | 11.05 | 10.80 | 9.94 | 9.36 | 10.2 | ~ | 756 | 3 |
| 9 | NAME LMC | G | 05 23 34.6 | -69 45 22 | 0.4 | ~ | 19090 | 0 | ||||
| 10 | NGC 2403 | AGN | 07 36 51.3381434280 | +65 36 09.650825640 | 9.31 | 8.84 | 8.38 | 8.19 | ~ | 1887 | 1 | |
| 11 | NGC 2903 | AGN | 09 32 10.111 | +21 30 02.99 | 10.44 | 9.75 | 9.07 | 8.68 | ~ | 1204 | 3 | |
| 12 | M 82 | AGN | 09 55 52.430 | +69 40 46.93 | 9.61 | 9.30 | 8.41 | ~ | 6156 | 6 | ||
| 13 | NGC 3310 | AGN | 10 38 45.85707 | +53 30 11.8940 | 12.45 | 12.15 | ~ | 809 | 1 | |||
| 14 | NGC 3628 | LIN | 11 20 17.018 | +13 35 22.16 | 10.42 | 9.48 | 9.22 | ~ | 853 | 3 | ||
| 15 | M 100 | AGN | 12 22 54.9299993592 | +15 49 20.296257960 | 10.04 | 10.05 | 9.35 | ~ | 1963 | 2 | ||
| 16 | NGC 4449 | EmG | 12 28 11.118 | +44 05 36.81 | 10.11 | 9.98 | 9.64 | 9.45 | ~ | 1192 | 1 | |
| 17 | NGC 4490 | GiG | 12 30 34.5 | +41 38 26 | 10.03 | 10.22 | 9.79 | ~ | 616 | 3 | ||
| 18 | CXOHDFN J123637.1+621135 | EmG | 12 36 36.8615 | +62 11 35.176 | 21.76 | 18.8662 | 20.7111 | 17.66 | 18.0676 | ~ | 45 | 0 |
| 19 | NAME SMM J123650+621316 | EmG | 12 36 49.74 | +62 13 13.0 | 25.47 | 23.7701 | 23.48 | 21.46 | 21.6273 | ~ | 89 | 1 |
| 20 | M 58 | Sy2 | 12 37 43.59747 | +11 49 05.1240 | 10.80 | 10.48 | 9.66 | ~ | 1140 | 2 | ||
| 21 | NGC 4631 | GiC | 12 42 08.009 | +32 32 29.44 | 9.78 | 9.19 | 9.10 | ~ | 1154 | 3 | ||
| 22 | NGC 4654 | H2G | 12 43 56.638 | +13 07 34.86 | 11.8 | ~ | 600 | 1 | ||||
| 23 | M 94 | SyG | 12 50 53.0737971432 | +41 07 12.900884628 | 9.15 | 8.96 | 8.24 | 7.78 | ~ | 1476 | 2 | |
| 24 | NGC 4945 | Sy2 | 13 05 27.279 | -49 28 04.44 | 9.31 | 14.40 | 7.55 | ~ | 1582 | 2 | ||
| 25 | M 83 | SBG | 13 37 00.91920 | -29 51 56.7400 | 8.85 | 8.11 | 7.52 | 7.21 | ~ | 2778 | 2 | |
| 26 | M 101 | GiP | 14 03 12.583 | +54 20 55.50 | 8.46 | 7.86 | 7.76 | ~ | 3138 | 2 | ||
| 27 | NAME Circinus Galaxy | Sy2 | 14 13 09.906 | -65 20 20.47 | 10.89 | 9.84 | 10.6 | 10.0 | ~ | 1331 | 1 | |
| 28 | NGC 6946 | H2G | 20 34 52.332 | +60 09 13.24 | 10.5 | ~ | 2661 | 2 | ||||
| 29 | NGC 7252 | AGN | 22 20 44.7748209648 | -24 40 41.909518200 | 12.26 | 12.46 | 12.06 | 11.57 | ~ | 720 | 1 |
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