Mid-infrared images of W75N (Persi+, 2006)

Bibcode
2007yCat..34450971P
Persi, P.; Tapia, M.; Smith, H. A.
Bibliographical reference

VizieR On-line Data Catalog: J/A+A/445/971. Originally published in: 2006A&A...445..971P

Advertised on:
2
2007
Number of authors
3
IAC number of authors
0
Citations
0
Refereed citations
0
Description
Mid-infrared images between 8.7 and 18.7um of W75N were taken during three observing runs on September 2000, November 2001 and September 2003 with the mid-infrared camera CID on the 2.1 m telescope of the Observatorio Astronomico Nacional at San Pedro Martir, Baja California, Mexico. The images at 3.6, 4.5, 5.8 and 8.0um of W75N presented here are sections of the original IRAC images of the star forming region DR21 observed during the science verification period of the Spitzer satellite. (1 data file).
Type
Non-refereed
H II regions
Infrared sources

It may interest you

  • Non-refereed
    Galaxy archaeology - The quest for ancient mergers
    The hierarchical assembly of galaxies through mergers is a key channel of galaxy evolution in the ΛCDM cosmological model. Quantifying these ancient transformative accretion events from observations of present day galaxies is a crucial goal of extragalactic archeology. Achieving this goal is challenging as the dominant epoch of galaxy assembly lies
    Ackerl, C. et al.

    Advertised on:

    3
    2024
    Bibcode
    2024aecc.conf....1A
    Citations
    0
  • Non-refereed
    RAD@home Citizen Scientists Uncover Emerging Jet-Galaxy Interactions
    The RAD12 object's recent investigation (Hota et al. 2022), via the RAD@home Astronomy Collaboratory, has provided a streamlined and focused perspective on the complex subject of jet-galaxy interactions, which has always posed a significant challenge for observational confirmation. This emerging field holds increasing significance, providing a
    Hota, Ananda et al.

    Advertised on:

    1
    2024
    Bibcode
    2024asi..confP..76H
    Citations
    0
  • Non-refereed
    A Disc Wind Where You Least Expect It: The Outflow in the Short-period X-ray Binary UW CrB
    Studying outflows of low mass X-ray binaries (LMXBs) is important for understanding the physics of accretion, the evolution of compact binaries, and dynamics of the local interstellar medium. One significant source of these outflows is the accretion disc wind, which can blow away vast amounts of material from the disc before it can be accreted on
    Fijma, Stefanie et al.

    Advertised on:

    5
    2024
    Bibcode
    2024HEAD...2150106F
    Citations
    0