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Query : 2018MNRAS.479.1866K |
2018MNRAS.479.1866K - Mon. Not. R. Astron. Soc., 479, 1866-1952 (2018/September-2)
An uncertainty principle for star formation - II. A new method for characterizing the cloud-scale physics of star formation and feedback across cosmic history.
KRUIJSSEN J.M.D., SCHRUBA A., HYGATE A.P.S., HU C.-Y., HAYDON D.T. and LONGMORE S.N.
Abstract (from CDS):
Abstract Copyright: © 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society
Journal keyword(s): stars: formation - ISM: evolution - galaxies: evolution - galaxies: formation - galaxies: ISM - galaxies: stellar content
Simbad objects: 7
Number of rows : 7 |
N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2024 |
#notes |
---|---|---|---|---|---|---|---|---|---|---|---|---|
1 | M 31 | AGN | 00 42 44.330 | +41 16 07.50 | 4.86 | 4.36 | 3.44 | ~ | 12651 | 1 | ||
2 | NGC 300 | GiG | 00 54 53.4465638304 | -37 41 03.168402396 | 8.83 | 8.69 | 8.13 | 7.46 | ~ | 1503 | 2 | |
3 | M 33 | GiG | 01 33 50.8965749232 | +30 39 36.630403128 | 6.17 | 6.27 | 5.72 | ~ | 5839 | 1 | ||
4 | NAME Magellanic Clouds | GrG | 03 00 | -71.0 | ~ | 7067 | 0 | |||||
5 | NAME LMC | G | 05 23 34.6 | -69 45 22 | 0.4 | ~ | 17438 | 0 | ||||
6 | M 51 | Sy2 | 13 29 52.698 | +47 11 42.93 | 9.26 | 8.36 | 8.40 | ~ | 4330 | 4 | ||
7 | NAME Local Group | GrG | ~ | ~ | ~ | 8393 | 0 |
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