IPHAS symbiotic stars candidates (Corradi+, 2008)

Bibcode
2008yCat..34800409C
Corradi, R. L. M.; Rodriguez-Flores, E. R.; Mampaso, A.; Greimel, R.; Viironen, K.; Drew, J. E.; Lennon, D. J.; Mikolajewska, J.; Sabin, L.; Sokoloski, J. L.
Bibliographical reference

VizieR On-line Data Catalog: J/A+A/480/409. Originally published in: 2008A&A...480..409C

Advertised on:
5
2008
Number of authors
10
IAC number of authors
0
Citations
0
Refereed citations
0
Description
As the present study was progressing, we started a campaign of spectroscopic follow-up of the Hα emitters detected by IPHAS. Accordingly a dozen candidate symbiotic stars, selected as described in the next sections, were observed at the INT using the IDS spectrograph, on nights of May 11, June 14, and September 9, 2006. (1 data file).
Type
Non-refereed
Surveys
Photometry

It may interest you

  • Non-refereed
    How 4MOST and MOONS will improve constraints on the dynamical masses of Local Group galaxies
    The wide-field spectrographs 4MOST and MOONS are expected to enter operations in late 2024 at the ESO Paranal Observatory. These upcoming survey facilities will play an important role in various fields over the next decade. In particular, both will host surveys aimed at observing Local Group (LG) galaxies. We describe how their scientific
    Mieske, S. et al.

    Advertised on:

    0
    2025
    Bibcode
    2025IAUS..379...49M
    Citations
    0
  • Non-refereed
    Star Formation History of the Small Magellanic Cloud: the shell-like structure
    We present the spatially resolved star formation history (SFH) of a shell-like structure located in the northeastern Small Magellanic Cloud (SMC). We quantitatively obtain the SFH using unprecedented deep photometric data (g ∼ 24 magnitude) from the SMASH survey and colour-magnitude diagram (CMD) fitting techniques. We consider, for the first time
    Sakowska, J. D. et al.

    Advertised on:

    0
    2025
    Bibcode
    2025IAUS..379..273S
    Citations
    0