Can gravitational waves be emitted from single neutron stars? I wonder whether GWs can be produced and emitted by single neutron stars, since it is known that typically they must be emitted by a binary system of them.
If so, can the source be an isolated cool neutron star or, for instance, a milisecond pulsar? I am an early learner on Neutron Star Physics, so I don't know if any neutron star itself can emit GWs. I once saw an open question (with no answer in the book) which asked if a single person would emit GWs by waving its own arms, and I couldn't help getting more confused.
I am also a bit aware with the quadrupole formula for compact objects, so I cannot see how a single star could contribute nonzero terms to it.
 A: Yes, single neutron stars can emit gravitational waves if they have sufficient asymmetries.
For some background, an object symmetric about its axis of rotation does not produce gravitational waves. A quote from Hartle's An Introduction to Einstein's General Relativity in the example "A Little Rotation" on page 497 of the textbook:

Axisymmetric rotation in general is an example of a highly symmetric motion that does not produce gravitational radiation.

For clarity, "axisymmetric" means "symmetric about an axis."
To view the details of the calculation, that section of Hartle is a good resource.
However, a rotating neutron star which does not have sufficient symmetry would emit gravitational waves. What's more, as pointed out by @Harti, pulsars must exhibit some sort of asymmetry in order to emit the radiation they do - but the question is whether these asymmetries are such that they will produce detectable gravitational waves.
As a concrete mathematical example of a neutron star that could emit gravitational waves, consider this problem written by an old professor of mine...

A neutron star of mass M and uniform mass density $\rho = 3M/4\pi\bar{R}^3$ has the shape of a slightly nonspherical ellipsoid, and rotates around its shortest $(z^\prime)$ axis with rotation period $P$. The lengths of the three principal axes $x^\prime, y^\prime, z^\prime$ (fixed in the body of the star) are in the ratios $(1+\epsilon) : 1 : (1+\epsilon)^{-1}$, where $\epsilon \ll 1$.
  
  
*
  
*Express the gravitational-wave luminosity of this object $(L_{GW})$ in terms of the quantities given above.
  
*Estimate the root-mean-square value of a component of $h_{ij}^{TT}$ of the strain at distance D from the star in terms of $L_{GW}$. (Ignore the dependence on the angle between the line of sight and the rotation axis.)
  
*Taking $M=1.4M_\odot$, $R = 10 \,\mathrm{km}$, $P = 1 \,\mathrm{ms}$, and $D = 10 \,\mathrm{kpc}$, estimate $\epsilon$ in order that $\langle(h_{ij}^{TT})^2\rangle^{1/2} \approx 10^{-23}$, the approximate current sensitivity of LIGO.
  

Understanding the solution would require some decent GR knowledge, but the point here is that, in principle, a single rotating body could emit gravitational radiation.
I am not sure if the particular scenario in the above problem is realistic, but it turns out that rotating neutron stars emitting gravitational waves is a realistic thing. See this article on astrobites about hunting for gravitational waves from spinning neutron stars.
A quote from the article that reinforces the above:

However, a neutron star must exhibit certain properties for it to be
  detectable through gravitational waves. A perfectly spherically
  symmetric neutron star won’t produce continuous gravitational waves as
  it rotates – the neutron star needs to maintain a long-lasting
  asymmetry. More importantly, this asymmetric distortion cannot be
  aligned with respect to the rotation axis (non-axisymmetric).

One example they mention is if the neutron star has some mountain on its surface.
(Note however that gravitational waves from single neutron stars have not yet been detected.)
A: In the regime of the quadrupole approximation, a body emits gravitational waves only if there is a change in its quadrupole moment. A perfectly spherical neutron star rotating symmetrically about its axis will not have any change in quadrupole moment and hence will not emit gravitational waves. However if the rotation is not symmetric about the axis, they will certainly emit gravitational waves, the intensity will probably depend on the extent of asymmetry.  
Pulsars beam em radiation and hence are not symmetric, therefore expected to produce gravitational radiation. Quoting Schutz (A First Course in General Relativity) - " Stars could radiate gravitational waves if they are not symmetric about the rotation axis. Pulsars are clearly not symmetric, since they beam their radiation somehow. But it is not clear how much mass asymmetry is required to produce the beaming."
Gravitational radiation emitted by binary neutron stars are in the detection range of our ground based detectors (LIGO, VIRGO) and hence the detection was possible. If the frequency of gravitational radiation of a spinning neutron star happens to be in the detection range and if the signal is "loud" enough, we may very well detect them ! 
