The spectral energy distribution of quiescent black hole X-ray binaries: new constraints from Spitze
Elena Gallo(University of Michigan–Ann Arbor), J. C. A. Miller‐Jones(Curtin University), Rob Fender(University of Southampton), Sera Markoff(University of Amsterdam), S. Berta(Institut de Radioastronomie Millimétrique), S. Migliari(University of California San Diego), Charles D. Bailyn(Yale University), John A. Tomsick(University of California, Berkeley)
Dipòsit Digital de la Universitat de Barcelona (Universitat de Barcelona)
November 1, 2007
Cited by 66
Related Papers
THE LESSER ROLE OF STARBURSTS IN STAR FORMATION AT <i>z</i> = 2
|The Astrophysical Journal Letters|2011|864
GALAXY STRUCTURE AND MODE OF STAR FORMATION IN THE SFR-MASS PLANE FROM<i>z</i>∼ 2.5 TO<i>z</i>∼ 0.1
|The Astrophysical Journal|2011|744
COMBINED CO AND DUST SCALING RELATIONS OF DEPLETION TIME AND MOLECULAR GAS FRACTIONS WITH COSMIC TIME, SPECIFIC STAR-FORMATION RATE, AND STELLAR MASS
|The Astrophysical Journal|2015|632
GMASS ultradeep spectroscopy of galaxies at<i>z</i>~ 2
|Astronomy and Astrophysics|2008|509
The Herschel★ PEP/HerMES luminosity function – I. Probing the evolution of PACS selected Galaxies to z ≃ 4
|Monthly Notices of the Royal Astronomical Society|2013|449