Andromeda's tenuous veil: A likely Milky Way nebula projected toward M3
Artikel i vetenskaplig tidskrift, 2025
Context. A large, faint nebula was unexpectedly discovered near M31 using narrowband [O III] images. Its apparent size and the lack of a clear counterpart at other wavelengths make it unique and challenging to explain. Aims. We aim to determine whether the nebula is extragalactic and vast or associated with the Milky Way filamentary structure. This will enable us to constrain its physical properties and assess its nature. Methods. We obtained deep narrowband [O II]3727 and Hα+[NII] observations with the JAST80 telescope at the Observatorio Astrofísico de Javalambre, as well as high spectral resolution spectroscopy (R ~ 5000) at four locations within the region of interest using the MEGARA integral field unit at the Gran Telescopio Canarias. Results. We found extended [O II] emission along two near-parallel strands to the [O III], offset by six arcmin. The nebular spectra reveal up to six emission lines from [O III]4959,5007, Hβ, [N II]6583, and [S II]6716,6731. Their receding velocities are above −40 km s−1, far from the systemic velocity of M31 (−300 km s−1). The fluxes and velocities are remarkably consistent for the same lines across different regions of the nebula. Conclusions. The nebular properties suggest a location within the Milky Way rather than being physically associated with M31. The most likely scenario suggests a resolved ionization structure in a Galactic nebula with a separation between [O II] and [O III] on the order of a few parsecs. The observed receding velocities would be unprecedented for an object physically linked to M31 but are common for nearby gas filaments. Their consistency across the nebula would also be highly unusual if it were larger than a kiloparsec. The analysis of the emission line ratios, line widths, and morphology suggests the possibility of it being an interstellar gas filament with an additional source of ionization to explain the [O III] emission. However, the complex properties of this object call for further observations to confirm its nature.
ISM: general
ISM: lines and bands
galaxies: individual: M31
ISM: kinematics and dynamics
ISM: clouds
Författare
A. Lumbreras-Calle
Centro de Estudios de Física del Cosmos de Aragón
J. A. Fernández-Ontiveros
Centro de Estudios de Física del Cosmos de Aragón
Centro de Estudios de Física del Cosmos de Aragón (CEFCA)
R. Infante-Sainz
Centro de Estudios de Física del Cosmos de Aragón
M. Akhlaghi
Centro de Estudios de Física del Cosmos de Aragón (CEFCA)
Centro de Estudios de Física del Cosmos de Aragón
Borja Montoro Molina
Consejo Superior de Investigaciones Científicas (CSIC)
Chalmers, Rymd-, geo- och miljövetenskap, Onsala rymdobservatorium
B. Pérez-Díaz
Consejo Superior de Investigaciones Científicas (CSIC)
A. Del Pino
Centro de Estudios de Física del Cosmos de Aragón
Consejo Superior de Investigaciones Científicas (CSIC)
Centro de Estudios de Física del Cosmos de Aragón (CEFCA)
H. Vives-Arias
Centro de Estudios de Física del Cosmos de Aragón
A. Hernán-Caballero
Centro de Estudios de Física del Cosmos de Aragón
Centro de Estudios de Física del Cosmos de Aragón (CEFCA)
C. López-Sanjuan
Centro de Estudios de Física del Cosmos de Aragón (CEFCA)
Centro de Estudios de Física del Cosmos de Aragón
M. A. Guerrero
Consejo Superior de Investigaciones Científicas (CSIC)
S. Eskandarlou
Centro de Estudios de Física del Cosmos de Aragón
A. Ederoclite
Centro de Estudios de Física del Cosmos de Aragón
Centro de Estudios de Física del Cosmos de Aragón (CEFCA)
Astronomy and Astrophysics
0004-6361 (ISSN) 1432-0746 (eISSN)
Vol. 704 A224Ämneskategorier (SSIF 2025)
Astronomi, astrofysik och kosmologi
DOI
10.1051/0004-6361/202453413