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Editorial25 March 2022
Editorial: Galactic Dynamics in the Solar Neighborhood

Editorial Article

Editorial: Galactic Dynamics in the Solar Neighborhood

Jacques R.D.Lepine

Departamento de Astronomia

Instituto de Astronomia, Geofísica e Ciências Atmosfericas

Universidade de São Paulo

This volume of Frontiers in Astronomy brings 6 interesting articles on the spiral structure of the Galaxy and on the stellar dynamics in the solar neighborhood. The spiral structure presented by Hektor Monteiro et al, derived from open clusters with astrometric positions from GAIA DR2 , and the one by Ligang Hou, based on giant molecular clouds, high-mass star-formation region masers, HII regions, and O stars , both in this volume, have similar results. There is no more doubt about the position of the arms in the solar neighborhood. The arms that we see in this region are the most visible part of the complete galactic arms structure, as revealed by VLBI maser observations that were published in recent years. The VLBI sources show that the Milky Way has a grand design spiral structure with 4 arms, that are about equally spaced, at least in the Galactic quadrants containing the Solar neighborhood. It is a little surprising that this better knowledge of the geometry of the arms has not been followed by a consensus concerning the physics or nature of the spiral arms. It seems that the Galactic Dynamics community is divided in two main tendencies: 1) those who believe that the spiral arms are long lived (a few billion years), and 2) those who think that the arms are short lived (about hundred Myr). However, there is not a real debate going on about this important question.

The corotation radius is the radial distance from the Galactic center at which the rotation curve of the material of the disk (gas, stars) rotate at the same velocity of the spiral arms. For the followers of the intermittent behavior of the arms, the corotation radius is not an interesting parameter. Corotation can be anywhere, many corotation radii can exist simultaneously. For the followers of the long-lived arms hypothesis, the corotation radius has a fundamental importance, since it is the location of the strongest resonance of the Galactic disk.

The question, then, comes about: is there something special at the corotation radius that is effectively observed? The answer comes by means of a technique which is quite simple, much used in Celestial Mechanics, but most often ignored in Galactic Dynamics. Since we have precise measurements of stellar positions and space velocities provided by GAIA DR2 and DR3, for millions of stars situated within a distance of about 2 kpc from the Sun, all what is needed to integrate the orbits of the stars is available. You can discover for each star if its orbit is normal (well behaved) or chaotic (departs strongly from the expected path). This is the technique of Dynamic Maps (Barros et al. in this volume). It is known from Celestial Mechanics that there is a concentration of chaotic stars at the frontiers of a resonance region. A strong resonance can be seen in the dynamic maps of the Solar neighborhood. Its position almost coincides with the solar radius. A direct determination of the spiral pattern speed, based on the birthplace of open clusters, (Monteiro et al., this volume) shows that the corotation is at this same radius.

Is this enough to settle the debate? No! First, there is many papers (tens of them) that attribute the dynamical anomaly to a resonance of the Galactic bar. without consensus on what resonance exactly is the best choice. For a given choice, the authors adjust the rotation speed of the bar, so that the chosen resonance happens to be at the Solar radius. A weakness of these models is that there is no independent measurement of the bar rotation speed to support their choice. Also, there are two well behaved spiral arms, Sagittarius-Carina and Scutum, between the extremity of the bar and the Sun, that do not seem to be perturbed by the potential of the bar. This puts limits on the strength of the bar. Second, another type of phenomenon, has been added to the list of candidates to produce anomalies in the solar vicinity: the infalling clouds or dwarf galaxies that may have reached the Galactic disk in a recent past.

These ideas are the consequence of an influential paper published in the journal Nature some 2 years ago, in which the authors claim to have discovered a kind of spiral structure in phase space including the Z direction. There was only one paper expressing some doubts about the reality of this spiral structure, while tens of papers accepted it as real and discussed different possibilities of infalling objects.

Finally, as another line of attack against the well-behaved grand design picture of the Galaxy, some work claim that there are arms that rotate with different velocities. If true, this would kill the grand design and long-lived picture. There cannot be strong spiral arms rotating at different velocities because the epicycle frequency can have only one value at a given radius, and the rotation speed of the arms is a combination of the frequency of the rotation curve and frequency of the epicycle.

In summary, nowadays, some authors believe that the Galaxy has a grand design style, and others believe that it is more like a flocculent Galaxy. New ways of thinking are needed. In their review on Astrochemistry, Edgar Mendoza et al. (this volume) shows in their section 2 that the presence of a step in the metallicity distribution in the Galactic disk is an indication of a long-lived structure. Amores & Levenhagen (this volume) suggest a new way, still in a preliminary development, to precisely map the spiral arms and the stellar population contained in them.

It seems it may be too early to say if a revival of the old theory of Marochnik, concerning the very narrow belt of life where we are, described in the last section of Barros et al. (this volume) will happen.

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The Spiral Structure in the Solar Neighborhood
REVIEW
6 August 2021
The Spiral Structure in the Solar Neighborhood
L. G. Hou
The spiral structure in the Solar neighborhood is an important issue in astronomy. In the past few years, there is significant progress in observation. The distances for a large number of good spiral tracers, i.e. giant molecular clouds, high-mass star-formation region masers, $\hii$ regions, O-type stars and young open clusters, have been accurately estimated, making it possible to depict the detailed properties of nearby spiral arms. In this work, we first give an overview about the research status for the Galaxy's spiral structure based on different types of tracers. Then the objects with distance uncertainties better than 15\% and $<$0.5~kpc are collected and combined together to depict the spiral structure in the Solar neighborhood. Five segments related with the Perseus, Local, Sagittarius-Carina, Scutum-Centaurus and Norma Arms are traced. With the large dataset, the parameters of the nearby arm segments are fitted and updated. Besides the dominant spiral arms, some substructures probably related to arm spurs or feathers are also noticed and discussed.

8,368 views

36 citations

The Distribution of Open Clusters in the Galaxy
In this work we explore the new catalog of galactic open clusters that became available recently, containing 1750 clusters that have been re-analysed using the Gaia DR2 catalog to determine the stellar memberships. We used the young open clusters as tracers of spiral arms and determined the spiral pattern rotation speed of the Galaxy and the corotation radius, the strongest Galactic resonance. The sample of open clusters used here increases the last one from Dias et al. (2019) used in the previous determination of the pattern speed by dozens objects. In addition, the distances and ages values are better determined, using improvements to isochrone fitting and including an updated extinction polynomial for the Gaia DR2 photometric band-passes, and the Galactic abundance gradient as a prior for metallicity. In addition to the better age determinations, the catalog contains better positions in the Galactic plane and better proper motions. This allow us to discuss not only the present space distribution of the clusters, but also the space distribution of the clusters's birthplaces, obtained by integration of the orbits for a time equal to their age. The value of the rotation velocity of the arms ($28.5 \pm 1.0$ km\,s$^{-1}$\,kpc$^{-1}$) implies that the corotation radius ($R_c$) is close to the solar Galactic orbit ($R_c/R_0 = 1.01\pm0.08$), which is supported by other observational evidence discussed in this text. A simulation is presented, illustrating the motion of the clusters in the reference frame of corotation. We also present general statistics of the catalog of clusters, like spatial distribution, distribution relative to height from the Galactic plane, and distribution of ages and metallicity. An important feature of the space distribution, the corotation gap in the gas distribution and its consequences for the young clusters, is discussed.

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28 citations

REVIEW
28 May 2021
Interrelations Between Astrochemistry and Galactic Dynamics
Edgar Mendoza, 5 more and Lars-Åke Nyman

6,994 views

3 citations

Dynamics of the Spiral-Arm Corotation and Its Observable Footprints in the Solar Neighborhood
REVIEW
20 April 2021
Dynamics of the Spiral-Arm Corotation and Its Observable Footprints in the Solar Neighborhood
Douglas A. Barros, 2 more and Jacques R. D. Lépine

6,498 views

12 citations