-
becoming Ultra Luminous Infrared Galaxys (
ULIRGs) but
there is no
perfect timetable because not all
LIRGs turn into
ULIRGs,
Newtonian mechanics is used in the...
-
sources of
ULIRGs in
general has been
greatly debated.
Infrared light from
galaxies generally originates from dust in the
interstellar medium.
ULIRGs are abnormally...
- ****ociated with
ULIRGs. It is not
known for sure that the UV
radiation is
produced purely by star-formation, and some
astronomers believe ULIRGs to be powered...
- Hasinger, G.; Leibundgut, B. (eds.). "Ultraviolet-Bright, High-Redshift
ULIRGS".
Relativistic Astrophysics Legacy and
Cosmology - Einstein's Legacy. Berlin...
-
formation rate of at
least 18 M☉ yr−1. Ultra-luminous
infrared galaxies (
ULIRGs) are at
least ten
times more
luminous still and form
stars at
rates >180 M☉ yr−1...
- "Optical
spectroscopy of Arp220: the star
formation history of the
closest ULIRG".
Monthly Notices of the
Royal Astronomical Society. 384 (3): 875–885. arXiv:0711...
-
GENERAL THEORY OF TURBULENCE-REGULATED STAR FORMATION, FROM
SPIRALS TO
ULIRGS".
Physics Department,
University of California, Berkeley, Berkeley, CA 94720...
- and by the
newly forming stars. APM is an ultra-luminous
infrared galaxy (
ULIRG). Its high
redshift shifts the far-infrared
spectrum into
millimeter wavelengths...
- and Radio-to-far-ultraviolet
Spectral Energy Distribution Modeling of 14
ULIRGs:
Insights into the
Global Properties of
Infrared Bright Galaxies". The Astrophysical...
-
Observations of the Gas-rich Host
Galaxy of PDS 456: A New
Challenge for the
ULIRG-to-QSO
Transition Scenario". The
Astrophysical Journal. 601 (2): 723–734...
