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I have read that it's not necessary for angular momentum and angular velocity to be parallel, but it is necessary for linear momentum and linear velocity to be parallel. How is this correct?

Note that this answer, like the tags of the question, is only focusing on Newtonian mechanics.

The definition of linear momentum $mathbf p$ is expressed in terms of the linear velocity $mathbf v$ using
$$mathbf p=mmathbf v$$
Since $m$ is just a scalar quantity, the vectors $mathbf p$ and $mathbf v$ are obviously parallel. i.e.
$$p_x=mv_x$$
$$p_y=mv_y$$
$$p_z=mv_z$$

However, the angular momentum $mathbf L$ is related to the angular velocity $boldsymbol omega$ by
$$mathbf L=mathbf Iboldsymbolomega$$

where $mathbf I$ is the moment of inertia tensor. This is explicitly written out as

$$
beginbmatrix
L_x\L_y\L_z
endbmatrix=
beginbmatrix
I_xx&I_xy&I_xz\
I_yx&I_yy&I_yz\
I_zx&I_zy&I_zz
endbmatrix
beginbmatrix
omega_x\omega_y\omega_z
endbmatrix
$$
Or each component written out:
$$L_x=I_xxomega_x+I_xyomega_y+I_xzomega_z$$
$$L_y=I_yxomega_x+I_yyomega_y+I_yzomega_z$$
$$L_z=I_zxomega_x+I_zyomega_y+I_zzomega_z$$

This shows that, in general, $mathbf L$ and $boldsymbolomega$ are not parallel. We have something more complicated than the linear case because each component of the angular momentum vector depends on all of the angular velocity components.

However, this complexity does not prevent our two vectors from being parallel. We can determine when they are parallel by looking at the equation
$$mathbf L=mathbf Iboldsymbolomega=Iboldsymbolomega$$
where $I$ is a scalar quantity. What this means is that $boldsymbolomega$ needs to be an eigenvector of $mathbf I$ in order for $mathbf L$ and $boldsymbolomega$ to be parallel. Note that this is usually what you encounter in your introductory physics classes. You, without knowing it, pick axes in such a way that the moment of inertia tensor is diagonal and your angular velocity is only along a single eigenvector (usually taken to be along the z-axis). For example, for a cylinder of radius $R$, height $H$, and mass $M$ rotating about its central axis aligned with the z-axis, we have
$$
beginbmatrix
L_x\L_y\L_z
endbmatrix=
beginbmatrix
frac112Mleft(3R^2+H^2right)&0&0\
0&frac112Mleft(3R^2+H^2right)&0\
0&0&frac12MR^2
endbmatrix
beginbmatrix
0\0\omega_z
endbmatrix
$$
Therefore we end up with the simple
$$mathbf L=L_zhat z=I_zzomega_zhat z=frac12MR^2omega_zhat z$$
or you might even see in an introductory physics class just
$$L=frac12MR^2omega$$

As a small note, the reason things become so much more complicated with the rotations is that the angular momentum not only depends on the mass of the object, but also how that mass is distributed. This is evident from the definition of angular momentum for a point particle $mathbf L=mathbf rtimesmathbf p$

However, if we look at an extended body's momentum we just get
$$mathbf p_T=m_Tmathbf v_textcom$$
where the $T$ subscript stands for "total" and "com$ is center of mass. Therefore, we still end up with a scalar mass instead of a tensor.

The other answers that say the difference arises because there is an inertia tensor in the rotation case are all perfectly correct, but i think we can go deeper and more intuitive that this and say:

Translations commute. Rotations don’t. That’s the fundamental reason for the difference. And it’s that way that these two different behaviors bear upon Noether’s theorem gives root to the difference between linear momentum, with its simple, scalar multiple relationship with velocity and angular momentum, with its more general linear transformation from the angular velocity vector.

Actually, the statement "Translations commute. Rotations don’t“ is a little glib and imprecise. But it's very close to being accurate. To be more precise, one would say rotations form a more complicated, noncommutative Lie group, whereas translations form „the" three dimensional commutative Lie group (commutative Lie groups of a given dimension are essentially all the same - there can be a topological difference in that the mutually commuting one parameter groups can be compact or not, but from the Lie algebra standpoint they are all exactly the same, and Noether’s theorem is only influenced by the Lie algebra, not by the group topology).

Recall that the reason for being for angular and linear momentum - what makes them useful concepts - is that they are conserved quantities of a physical system (in the absence of external forces). And, although Noether’s theorem is not the only mechanism that gives rise to conserved quantities in physics, it is in this case. So, if we want fundamental, intuitive insight into this question, we must look at how Noether’s theorem plays out in the two cases.

Let’s grab the expression from Wikipedia for the conserved Noether current:

$$left(fracpartial Lpartial dotmathbfq cdot dotmathbfq - L right) T_r - fracpartial Lpartial dotmathbfq cdot mathbfQ_rtag1$$

This is a very physicist equation and needs explanation if you’re not familiar with its notation and jargon. Noether’s theorem states that if the Lagrangian of a system is time-translation-invariant and is invariant with respect to a continuous, one-parameter group of transformations on the system’s generalized co-ordinates, then there is a conserved quantity for each such one parameter group, called to Noether charge. For example: rotations of the co-ordinate system about an axis - the rotation’s magnitude can be smoothly varied with the rotation angle - or translations along a given direction of the co-ordinate origin, which are parameterized by a 1continuous signed distance value. In (1), $mathbfQ_r$ is the „generator" of the continuous transformation in question (explained below). The first part of (1) - the bit to the left of $T_r$, has to do with the continuous transformation of translating the time co-ordinate, and is not important for the present considerations. It gives rise to the energy as a c1onserved quantity. So we look at the part that is nonzero for the transformations (on the non-time co-ordinates) that we’re interested in:

$$fracpartial Lpartial dotmathbfq cdot mathbfQ_rtag2$$

As someone versed in a more Lie theoretical understanding of these matters, i would write the above equation more to my taste as follows:

$$mathbfQ_r fracpartial Lpartial dotmathbfq = mathbfQ_r , mathbfptag3$$

where $fracpartial Lpartial dotmathbfq$ is a vector whose components are the generalized momenta $p_i = fracpartial Lpartial dotq_i$ corresponding to the generalized co-ordinates $p_i$ of the Lagrangian description. In the above, $mathbfQ_r$ is the matrix of the Lie algebra member when the Lie group in question acts on the generalized co-ordinates.

So, let’s see how (3) pans out. If our Lagrangian is independent of the generalized co-ordinates themselves, then the matrix of the translation in the $i^th$ direction is simply diagonal with noughts along its leading diagonal except at the $i^th$ position. So (3) just says that the $i^th$ component of the generalized momentum $mathbfp$ is conserved. Or, repeating the argument for each $i$, the $mathbfp$ itself is conserved. So the situation is very simple for translations in the co-ordinates themselves.

However, if the concept of rotation of generalized co-ordinates is meaningful, and, if further, the Lagrangian is invariant with respect to rotations in the generalized co-ordinates, then the matrix $mathbfQ_r$ in (3) is the Lie algebra member of $SO(N)$ corresponding to rotation about the axis in question, times the distance $r$ from the co-ordinate origin (this is the $N$-dimensional generalization corresponding to the vector calculus operator $mathbfomegatimesmathbfr$ in 3 dimensions). So already, without assuming anything about the expressions for angular or linear momentum aside from that our Lagrangian is invariant to translations and rotations, we can see that the expressions for the conserved linear momentums are simply the generalized momentums themselves, whereas the conserved angular momentums, by dent of the more complicated Lie algebra for $SO(N)$ are matrix operations on the generalized momentums.

If we further assume that the generalized momentum is $m_i,r, mathbfQ_r dottheta_r$ (the $N$-dimensional generalization corresponding to the vector calculus expression $mathbfomegatimes mathbfr$ in 3 dimensions), then our Noether charge is:

$$m ,r^2 ,mathbfQ_r^2 dottheta_rtag5$$

and this quantity is conserved for each co-ordinate $r$. This is readily shown to mean the same thing as the conservation of $mathbfL = mathbfI,mathbfomega$ when summed over all particles in a rigid body.

Actually, i believe my answer above is the fundamental grounds for Aaron Stevens' excellent physical intuition::

As a small note, the reason things become so much more complicated with the rotations is that the angular momentum not only depends on the mass of the object, but also how that mass is distributed.

Mass is a scalar but mass moment of inertia is a tensor. As a result, a scalar can only change the magnitude of a vector, but a tensor can change both the magnitude and the direction.

From linear algebra:

• 
  $boldsymbolp = m boldsymbolv$ is always parallel to $boldsymbolv$ for $m neq 0$
  


• 
  $boldsymbolL = rmI, boldsymbolomega$ is only parallel when $boldsymbolomega$ is an eigenvector of $mathrmI$. A special case exists for symmetric objects like spheres and cubes where $mathrmI$ is a scalar multiple of the identity matrix.

Linear momentum is defined as

$$vecp=mvecv$$

where $m$ is a scalar (i.e. just a number). Multiplying a vector by a scalar does not change its direcction.

In contrast, angular momentum is defined as

$$vecL=oversetleftrightarrowIvecomega$$

where $oversetleftrightarrowI$ is a tensor (i.e. something like, but not quite exactly, a matrix). Multiplying a vector by a tensor can, and often does, change the direction of the vector.