TY - JOUR
T1 - Young, Blue, and Isolated Stellar Systems in the Virgo Cluster. I. 2D Optical Spectroscopy
AU - Bellazzini, Michele
AU - Magrini, Laura
AU - Jones, Michael G.
AU - Sand, David J.
AU - Beccari, Giacomo
AU - Cresci, Giovanni
AU - Spekkens, Kristine
AU - Karunakaran, Ananthan
AU - Adams, Elizabeth A.K.
AU - Zaritsky, Dennis
AU - Battaglia, Giuseppina
AU - Seth, Anil
AU - Cannon, John M.
AU - Fuson, Jackson
AU - Inoue, John L.
AU - Mutlu-Pakdil, Burçin
AU - Guhathakurta, Puragra
AU - Muñoz, Ricardo R.
AU - Bennet, Paul
AU - Crnojević, Denija
AU - Caldwell, Nelson
AU - Strader, Jay
AU - Toloba, Elisa
N1 - Publisher Copyright:
© 2022. The Author(s). Published by the American Astronomical Society.
PY - 2022/8/1
Y1 - 2022/8/1
N2 - We use panoramic optical spectroscopy obtained with the Very Large Telescope/MUSE to investigate the nature of five candidate extremely isolated low-mass star-forming regions (Blue Candidates; hereafter, BCs) toward the Virgo cluster of galaxies. Four of the five (BC1, BC3, BC4, and BC5) are found to host several H ii regions and to have radial velocities fully compatible with being part of the Virgo cluster. All the confirmed candidates have mean metallicity significantly in excess of that expected from their stellar mass, indicating that they originated from gas stripped from larger galaxies. In summary, these four candidates share the properties of the prototype system SECCO 1, suggesting the possible emergence of a new class of stellar systems, intimately linked to the complex duty cycle of gas within clusters of galaxies. A thorough discussion of the nature and evolution of these objects is presented in a companion paper, where the results obtained here from the MUSE data are complemented with Hubble Space Telescope (optical) and Very Large Array (Hi) observations.
AB - We use panoramic optical spectroscopy obtained with the Very Large Telescope/MUSE to investigate the nature of five candidate extremely isolated low-mass star-forming regions (Blue Candidates; hereafter, BCs) toward the Virgo cluster of galaxies. Four of the five (BC1, BC3, BC4, and BC5) are found to host several H ii regions and to have radial velocities fully compatible with being part of the Virgo cluster. All the confirmed candidates have mean metallicity significantly in excess of that expected from their stellar mass, indicating that they originated from gas stripped from larger galaxies. In summary, these four candidates share the properties of the prototype system SECCO 1, suggesting the possible emergence of a new class of stellar systems, intimately linked to the complex duty cycle of gas within clusters of galaxies. A thorough discussion of the nature and evolution of these objects is presented in a companion paper, where the results obtained here from the MUSE data are complemented with Hubble Space Telescope (optical) and Very Large Array (Hi) observations.
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U2 - 10.3847/1538-4357/ac7c6d
DO - 10.3847/1538-4357/ac7c6d
M3 - Article
AN - SCOPUS:85136049789
SN - 0004-637X
VL - 935
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 1
M1 - 50
ER -