9 datasets found

Keywords: star forming regions

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  • Star formation properties of LSBGs and SFs

    We analyzed the star formation surface density ({SIGMA}SFR) between the global and HII regions in a sample of 69 low surface brightness galaxies (LSBGs) and 68 star-forming (SF)...
  • ALMA-IRDC from cloud to core scales

    Infrared dark clouds (IRDCs) are potential hosts of the elusive early phases of high mass star formation (HMSF). Here, we conduct an in-depth analysis of the fragmentation...
  • Star-forming Regions of NGC 7469

    We present James Webb Space Telescope (JWST) imaging of NGC 7469 with the Near-Infrared Camera (NIRCam) and the Mid-InfraRed Instrument (MIRI). NGC 7469 is a nearby, z=0.016317,...
  • Galaxy Zoo: Clump Scout: clumpy SDSS gal. at z~<0.2

    Massive, star-forming clumps are a common feature of high-redshift star-forming galaxies. How they formed, and why they are so rare at low redshift, remains unclear. In this...
  • 44GHz VLA obs. of methanol masers in DR21(OH)

    High-mass stars play an important role in the interstellar medium, but much remains to be known about their formation. Class I methanol masers may be unique tracers of an early...
  • Radial velocities in W5 YSO groups

    The star-forming region W5 is a major part of the Cassiopeia OB6 association. Its internal structure and kinematics may provide hints of the star formation process in this...
  • SFACT. III. SFF01 -10 and -15 spectral data

    The Star Formation Across Cosmic Time (SFACT) survey is a new narrowband survey designed to detect emission-line galaxies (ELGs) and quasi-stellar objects (QSOs) over a wide...
  • SFACT. II. SFF01 -10 and -15 emission line objects

    Star Formation Across Cosmic Time (SFACT) is a new narrowband (NB) survey designed to detect faint emission-line galaxies (ELGs) and QSOs over a broad range of redshifts. Here...
  • 6.7GHz methanol maser flare in G11.497-1.485

    Maser flares are of particular significance for the study of massive star formation as they not only signal but also provide unique insights into transient phenomena such as...
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